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Australian SKA Pathfinder
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if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="4346B9FAADAA764CB6B122FBBF5B1E56" data-container="representation" aria-label="Export citation for Unexpected circular radio objects at high Galactic latitude">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2020.52" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358020000521')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Unexpected circular radio objects at high Galactic latitude" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"4346B9FAADAA764CB6B122FBBF5B1E56"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358020000521" class="content"> <div class="abstract" data-abstract-type="normal"><p>We have found a class of circular radio objects in the Evolutionary Map of the Universe Pilot Survey, using the Australian Square Kilometre Array Pathfinder telescope. The objects appear in radio images as circular edge-brightened discs, about one arcmin diameter, that are unlike other objects previously reported in the literature. We explore several possible mechanisms that might cause these objects, but none seems to be a compelling explanation.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.52" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.52" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="4A1684E726FAE189CB1B1B918C47E005" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"4A1684E726FAE189CB1B1B918C47E005","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="4A1684E726FAE189CB1B1B918C47E005" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="1087937" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/gaskapthe-galactic-askap-survey/4A1684E726FAE189CB1B1B918C47E005"> GASKAP—The Galactic ASKAP Survey </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=John M. Dickey&eventCode=SE-AU" class="more-by-this-author ">John M. Dickey</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Naomi McClure-Griffiths&eventCode=SE-AU" class="more-by-this-author ">Naomi McClure-Griffiths</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Steven J. Gibson&eventCode=SE-AU" class="more-by-this-author ">Steven J. Gibson</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=José F. Gómez&eventCode=SE-AU" class="more-by-this-author ">José F. 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The survey will study the distribution of H <span class='sc'>i</span> emission and absorption with unprecedented angular and velocity resolution, as well as molecular line thermal emission, absorption, and maser lines. The area to be covered includes the Galactic plane (|<span class='italic'>b</span>| < 10°) at all declinations south of δ = +40°, spanning longitudes 167° through 360°to 79° at <span class='italic'>b</span> = 0°, plus the entire area of the Magellanic Stream and Clouds, a total of 13 020 deg<span class='sup'>2</span>. The brightness temperature sensitivity will be very good, typically σ<span class='sub'>T</span>≃ 1 K at resolution 30 arcsec and 1 km s<span class='sup'>−1</span>. The survey has a wide spectrum of scientific goals, from studies of galaxy evolution to star formation, with particular contributions to understanding stellar wind kinematics, the thermal phases of the interstellar medium, the interaction between gas in the disk and halo, and the dynamical and thermal states of gas at various positions along the Magellanic Stream.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2012.003" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2012.003" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="976D588E264A5ED16A5E7EA180F9FE02" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"976D588E264A5ED16A5E7EA180F9FE02","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="976D588E264A5ED16A5E7EA180F9FE02" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="497" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/sptcl-j20325627-a-new-southern-double-relic-cluster-observed-with-askap/976D588E264A5ED16A5E7EA180F9FE02"> SPT-CL J2032–5627: A new Southern double relic cluster observed with ASKAP </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=S. W. Duchesne&eventCode=SE-AU" class="more-by-this-author ">S. W. Duchesne</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=M. Johnston-Hollitt&eventCode=SE-AU" class="more-by-this-author ">M. Johnston-Hollitt</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=I. Bartalucci&eventCode=SE-AU" class="more-by-this-author ">I. Bartalucci</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=T. Hodgson&eventCode=SE-AU" class="more-by-this-author ">T. Hodgson</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=G. W. Pratt&eventCode=SE-AU" class="more-by-this-author ">G. W. Pratt</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/08A6F1C86EBBD90385E0EF1AF9272071" class="productParent" data-prod-id="08A6F1C86EBBD90385E0EF1AF9272071">Volume 38</a> / 2021 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 18 January 2021</span><span class="pages">, e005</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-976D588E264A5ED16A5E7EA180F9FE02" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/976D588E264A5ED16A5E7EA180F9FE02/S132335802000051Xa.pdf/sptcl_j20325627_a_new_southern_double_relic_cluster_observed_with_askap.pdf" data-pdf-content-id="976D588E264A5ED16A5E7EA180F9FE02" target="_blank" aria-label="Download PDF for SPT-CL J2032–5627: A new Southern double relic cluster observed with ASKAP [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/976D588E264A5ED16A5E7EA180F9FE02/core-reader" target="_blank" aria-label="View HTML full text for SPT-CL J2032–5627: A new Southern double relic cluster observed with ASKAP [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"976D588E264A5ED16A5E7EA180F9FE02","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="976D588E264A5ED16A5E7EA180F9FE02" data-container="representation" aria-label="Export citation for SPT-CL J2032–5627: A new Southern double relic cluster observed with ASKAP">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2020.51" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS132335802000051X')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for SPT-CL J2032–5627: A new Southern double relic cluster observed with ASKAP" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"976D588E264A5ED16A5E7EA180F9FE02"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS132335802000051X" class="content"> <div class="abstract" data-abstract-type="normal"><p>We present a radio and X-ray analysis of the galaxy cluster SPT-CL J2032–5627. Investigation of public data from the Australian Square Kilometre Array Pathfinder (ASKAP) at 943 MHz shows two previously undetected radio relics at either side of the cluster. For both relic sources, we utilise archival Australia Telescope Compact Array (ATCA) data at 5.5 GHz in conjunction with the new ASKAP data to determine that both have steep integrated radio spectra (<span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210115175235068-0377:S132335802000051X:S132335802000051X_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\ensuremath{{\alpha_\mathrm{SE} = -1.52 \pm 0.10}}$ </span></span></span></span> and <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210115175235068-0377:S132335802000051X:S132335802000051X_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\ensuremath{{\alpha_\mathrm{NW,full} = -1.18 \pm 0.10}}$ </span></span></span></span> for the southeast and northwest relic sources, respectively). No shock is seen in XMM-<span class='italic'>Newton</span> observations; however, the southeast relic is preceded by a cold front in the X-ray–emitting intra-cluster medium. We suggest the lack of a detectable shock may be due to instrumental limitations, comparing the situation to the southeast relic in Abell 3667. We compare the relics to the population of double relic sources and find that they are located below the current power–mass scaling relation. We present an analysis of the low-surface brightness sensitivity of ASKAP and the ATCA, the excellent sensitivity of both allow the ability to find heretofore undetected diffuse sources, suggesting these low-power radio relics will become more prevalent in upcoming large-area radio surveys such as the Evolutionary Map of the Universe.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.51" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.51" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="E4E1BEB867290973BCB7C28AB2C5E241" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"E4E1BEB867290973BCB7C28AB2C5E241","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="E4E1BEB867290973BCB7C28AB2C5E241" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="798004" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/vast-an-askap-survey-for-variables-and-slow-transients/E4E1BEB867290973BCB7C28AB2C5E241"> VAST: An ASKAP Survey for Variables and Slow Transients </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=TARA MURPHY&eventCode=SE-AU" class="more-by-this-author ">TARA MURPHY</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=SHAMI CHATTERJEE&eventCode=SE-AU" class="more-by-this-author ">SHAMI CHATTERJEE</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=DAVID L. 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WILLIAMS</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/DF38508038A251E724869CA9F573BAD5" class="productParent" data-prod-id="DF38508038A251E724869CA9F573BAD5">Volume 30</a> / 2013 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 15 February 2013</span><span class="pages">, e006</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-E4E1BEB867290973BCB7C28AB2C5E241" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/E4E1BEB867290973BCB7C28AB2C5E241/S1323358012000069a.pdf/vast_an_askap_survey_for_variables_and_slow_transients.pdf" data-pdf-content-id="E4E1BEB867290973BCB7C28AB2C5E241" target="_blank" aria-label="Download PDF for VAST: An ASKAP Survey for Variables and Slow Transients [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/E4E1BEB867290973BCB7C28AB2C5E241/core-reader" target="_blank" aria-label="View HTML full text for VAST: An ASKAP Survey for Variables and Slow Transients [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"E4E1BEB867290973BCB7C28AB2C5E241","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="E4E1BEB867290973BCB7C28AB2C5E241" data-container="representation" aria-label="Export citation for VAST: An ASKAP Survey for Variables and Slow Transients">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2012.006" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358012000069')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for VAST: An ASKAP Survey for Variables and Slow Transients" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"E4E1BEB867290973BCB7C28AB2C5E241"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358012000069" class="content"> <div class="abstract" data-abstract-type="normal"><p>The Australian Square Kilometre Array Pathfinder (ASKAP) will give us an unprecedented opportunity to investigate the transient sky at radio wavelengths. In this paper we present VAST, an ASKAP survey for Variables and Slow Transients. VAST will exploit the wide-field survey capabilities of ASKAP to enable the discovery and investigation of variable and transient phenomena from the local to the cosmological, including flare stars, intermittent pulsars, X-ray binaries, magnetars, extreme scattering events, interstellar scintillation, radio supernovae, and orphan afterglows of gamma-ray bursts. In addition, it will allow us to probe unexplored regions of parameter space where new classes of transient sources may be detected. In this paper we review the known radio transient and variable populations and the current results from blind radio surveys. We outline a comprehensive program based on a multi-tiered survey strategy to characterise the radio transient sky through detection and monitoring of transient and variable sources on the ASKAP imaging timescales of 5 s and greater. We also present an analysis of the expected source populations that we will be able to detect with VAST.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2012.006" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2012.006" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="BF7FC8D2E30F8F1CB698CBD084A02946" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"BF7FC8D2E30F8F1CB698CBD084A02946","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="BF7FC8D2E30F8F1CB698CBD084A02946" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="243" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/remnant-radio-galaxies-discovered-in-a-multifrequency-survey/BF7FC8D2E30F8F1CB698CBD084A02946"> Remnant radio galaxies discovered in a multi-frequency survey </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> <li><a href="/core/product/identifier/GAMA_LEGACY_ATCA_SOUTHERN_SURVEY_1/type/BESPOKE_COLLECTION" class="">GAMA Legacy ATCA Southern Survey </a></li> <li><a href="/core/product/identifier/DE297729-82B2-4EAF-A1E8-1150AB51579E/type/BESPOKE_COLLECTION" class="">Murchison Widefield Array</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Benjamin Quici&eventCode=SE-AU" class="more-by-this-author ">Benjamin Quici</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Natasha Hurley-Walker&eventCode=SE-AU" class="more-by-this-author ">Natasha Hurley-Walker</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Nicholas Seymour&eventCode=SE-AU" class="more-by-this-author ">Nicholas Seymour</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Ross J. 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if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="BF7FC8D2E30F8F1CB698CBD084A02946" data-container="representation" aria-label="Export citation for Remnant radio galaxies discovered in a multi-frequency survey">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2020.49" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358020000491')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Remnant radio galaxies discovered in a multi-frequency survey" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"BF7FC8D2E30F8F1CB698CBD084A02946"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358020000491" class="content"> <div class="abstract" data-abstract-type="normal"><p>The remnant phase of a radio galaxy begins when the jets launched from an active galactic nucleus are switched off. To study the fraction of radio galaxies in a remnant phase, we take advantage of a <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210208170753778-0421:S1323358020000491:S1323358020000491_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$8.31$</span></span></span></span> deg<span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210208170753778-0421:S1323358020000491:S1323358020000491_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$^2$</span></span></span></span> subregion of the GAMA 23 field which comprises of surveys covering the frequency range 0.1–9 GHz. We present a sample of 104 radio galaxies compiled from observations conducted by the Murchison Widefield Array (216 MHz), the Australia Square Kilometer Array Pathfinder (887 MHz), and the Australia Telescope Compact Array (5.5 GHz). We adopt an ‘absent radio core’ criterion to identify 10 radio galaxies showing no evidence for an active nucleus. We classify these as new candidate remnant radio galaxies. Seven of these objects still display compact emitting regions within the lobes at 5.5 GHz; at this frequency the emission is short-lived, implying a recent jet switch off. On the other hand, only three show evidence of aged lobe plasma by the presence of an ultra-steep-spectrum (<span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210208170753778-0421:S1323358020000491:S1323358020000491_inline3.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\alpha<-1.2$</span></span></span></span>) and a diffuse, low surface brightness radio morphology. The predominant fraction of young remnants is consistent with a rapid fading during the remnant phase. Within our sample of radio galaxies, our observations constrain the remnant fraction to <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210208170753778-0421:S1323358020000491:S1323358020000491_inline4.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$4\%\lesssim f_{\mathrm{rem}} \lesssim 10\%$</span></span></span></span>; the lower limit comes from the limiting case in which all remnant candidates with hotspots are simply active radio galaxies with faint, undetected radio cores. Finally, we model the synchrotron spectrum arising from a hotspot to show they can persist for 5–10 Myr at 5.5 GHz after the jets switch of—radio emission arising from such hotspots can therefore be expected in an appreciable fraction of genuine remnants.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.49" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.49" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="E1A1DC57B4850811F5624AD3E97C9C9E" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"E1A1DC57B4850811F5624AD3E97C9C9E","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="E1A1DC57B4850811F5624AD3E97C9C9E" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="352" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/australian-square-kilometre-array-pathfinder-i-system-description/E1A1DC57B4850811F5624AD3E97C9C9E"> Australian square kilometre array pathfinder: I. system description </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=A. 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Westmeier</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/08A6F1C86EBBD90385E0EF1AF9272071" class="productParent" data-prod-id="08A6F1C86EBBD90385E0EF1AF9272071">Volume 38</a> / 2021 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 05 March 2021</span><span class="pages">, e009</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-E1A1DC57B4850811F5624AD3E97C9C9E" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/E1A1DC57B4850811F5624AD3E97C9C9E/S1323358021000011a.pdf/australian_square_kilometre_array_pathfinder_i_system_description.pdf" data-pdf-content-id="E1A1DC57B4850811F5624AD3E97C9C9E" target="_blank" aria-label="Download PDF for Australian square kilometre array pathfinder: I. system description [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/E1A1DC57B4850811F5624AD3E97C9C9E/core-reader" target="_blank" aria-label="View HTML full text for Australian square kilometre array pathfinder: I. system description [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"E1A1DC57B4850811F5624AD3E97C9C9E","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); 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ASKAP is one of the first radio telescopes to deploy phased array feed (PAF) technology on a large scale, giving it an instantaneous field of view that covers <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210304142501921-0523:S1323358021000011:S1323358021000011_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$31\,\textrm{deg}^{2}$</span></span></span></span> at <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210304142501921-0523:S1323358021000011:S1323358021000011_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$800\,\textrm{MHz}$</span></span></span></span>. As a two-dimensional array of 36<span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210304142501921-0523:S1323358021000011:S1323358021000011_inline3.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\times$</span></span></span></span>12 m antennas, with baselines ranging from 22 m to 6 km, ASKAP also has excellent snapshot imaging capability and 10 arcsec resolution. This, combined with 288 MHz of instantaneous bandwidth and a unique third axis of rotation on each antenna, gives ASKAP the capability to create high dynamic range images of large sky areas very quickly. It is an excellent telescope for surveys between 700 and <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210304142501921-0523:S1323358021000011:S1323358021000011_inline4.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$1800\,\textrm{MHz}$</span></span></span></span> and is expected to facilitate great advances in our understanding of galaxy formation, cosmology, and radio transients while opening new parameter space for discovery of the unknown.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.1" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.1" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="79F8A6BC5B8219B11165FBEAAB2354E7" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"79F8A6BC5B8219B11165FBEAAB2354E7","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="79F8A6BC5B8219B11165FBEAAB2354E7" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="848807" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/measuring-noise-temperatures-of-phasedarray-antennas-for-astronomy-at-csiro/79F8A6BC5B8219B11165FBEAAB2354E7"> Measuring Noise Temperatures of Phased-Array Antennas for Astronomy at CSIRO </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=A. P. Chippendale&eventCode=SE-AU" class="more-by-this-author ">A. P. Chippendale</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=D. B. Hayman&eventCode=SE-AU" class="more-by-this-author ">D. B. Hayman</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=S. G. Hay&eventCode=SE-AU" class="more-by-this-author ">S. G. Hay</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/23650F62BEA6AC5730F9F3CF8131D599" class="productParent" data-prod-id="23650F62BEA6AC5730F9F3CF8131D599">Volume 31</a> / 2014 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 01 April 2014</span><span class="pages">, e019</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-79F8A6BC5B8219B11165FBEAAB2354E7" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/79F8A6BC5B8219B11165FBEAAB2354E7/S1323358014000113a.pdf/measuring_noise_temperatures_of_phasedarray_antennas_for_astronomy_at_csiro.pdf" data-pdf-content-id="79F8A6BC5B8219B11165FBEAAB2354E7" target="_blank" aria-label="Download PDF for Measuring Noise Temperatures of Phased-Array Antennas for Astronomy at CSIRO [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/79F8A6BC5B8219B11165FBEAAB2354E7/core-reader" target="_blank" aria-label="View HTML full text for Measuring Noise Temperatures of Phased-Array Antennas for Astronomy at CSIRO [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"79F8A6BC5B8219B11165FBEAAB2354E7","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="79F8A6BC5B8219B11165FBEAAB2354E7" data-container="representation" aria-label="Export citation for Measuring Noise Temperatures of Phased-Array Antennas for Astronomy at CSIRO">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2014.11" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358014000113')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Measuring Noise Temperatures of Phased-Array Antennas for Astronomy at CSIRO" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"79F8A6BC5B8219B11165FBEAAB2354E7"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358014000113" class="content"> <div class="abstract" data-abstract-type="normal"><p>We describe the development of a noise-temperature testing capability for phased-array antennas operating in receive mode from 0.7 GHz to 1.8 GHz. Sampled voltages from each array port were recorded digitally as the zenith-pointing array under test was presented with three scenes: (1) a large microwave absorber at ambient temperature, (2) the unobstructed radio sky, and (3) broadband noise transmitted from a reference antenna centred over and pointed at the array under test. The recorded voltages were processed in software to calculate the beam equivalent noise temperature for a maximum signal-to-noise ratio beam steered at the zenith. We introduced the reference-antenna measurement to make noise measurements with reproducible, well-defined beams directed at the zenith and thereby at the centre of the absorber target. We applied a detailed model of cosmic and atmospheric contributions to the radio sky emission that we used as a noise-temperature reference. We also present a comprehensive analysis of measurement uncertainty including random and systematic effects. The key systematic effect was due to uncertainty in the beamformed antenna pattern and how efficiently it illuminates the absorber load. We achieved a combined uncertainty as low as 4 K for a 40 K measurement of beam equivalent noise temperature. The measurement and analysis techniques described in this paper were pursued to support noise-performance verification of prototype phased-array feeds for the Australian Square Kilometre Array Pathfinder telescope.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2014.11" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2014.11" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="9DF3F1D3FFC020F1A9299444420D71D4" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"9DF3F1D3FFC020F1A9299444420D71D4","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="9DF3F1D3FFC020F1A9299444420D71D4" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="237" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/early-science-from-possum-shocks-turbulence-and-a-massive-new-reservoir-of-ionised-gas-in-the-fornax-cluster/9DF3F1D3FFC020F1A9299444420D71D4"> Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=C. 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Warhurst</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/08A6F1C86EBBD90385E0EF1AF9272071" class="productParent" data-prod-id="08A6F1C86EBBD90385E0EF1AF9272071">Volume 38</a> / 2021 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 23 April 2021</span><span class="pages">, e020</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-9DF3F1D3FFC020F1A9299444420D71D4" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/9DF3F1D3FFC020F1A9299444420D71D4/S1323358021000047a.pdf/early_science_from_possum_shocks_turbulence_and_a_massive_new_reservoir_of_ionised_gas_in_the_fornax_cluster.pdf" data-pdf-content-id="9DF3F1D3FFC020F1A9299444420D71D4" target="_blank" aria-label="Download PDF for Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/9DF3F1D3FFC020F1A9299444420D71D4/core-reader" target="_blank" aria-label="View HTML full text for Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"9DF3F1D3FFC020F1A9299444420D71D4","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="9DF3F1D3FFC020F1A9299444420D71D4" data-container="representation" aria-label="Export citation for Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2021.4" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358021000047')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"9DF3F1D3FFC020F1A9299444420D71D4"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358021000047" class="content"> <div class="abstract" data-abstract-type="normal"><p>We present the first Faraday rotation measure (RM) grid study of an individual low-mass cluster—the Fornax cluster—which is presently undergoing a series of mergers. Exploiting commissioning data for the POlarisation Sky Survey of the Universe’s Magnetism (POSSUM) covering a <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210422083154459-0643:S1323358021000047:S1323358021000047_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>${\sim}34$</span></span></span></span> square degree sky area using the Australian Square Kilometre Array Pathfinder (ASKAP), we achieve an RM grid density of <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210422083154459-0643:S1323358021000047:S1323358021000047_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>${\sim}25$</span></span></span></span> RMs per square degree from a 280-MHz band centred at 887 MHz, which is similar to expectations for forthcoming GHz-frequency <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210422083154459-0643:S1323358021000047:S1323358021000047_inline3.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>${\sim}3\pi$</span></span></span></span>-steradian sky surveys. These data allow us to probe the extended magnetoionic structure of the cluster and its surroundings in unprecedented detail. We find that the scatter in the Faraday RM of confirmed background sources is increased by <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210422083154459-0643:S1323358021000047:S1323358021000047_inline4.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$16.8\pm2.4$</span></span></span></span> rad m<span class='sup'>−2</span> within 1<span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210422083154459-0643:S1323358021000047:S1323358021000047_inline5.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$^\circ$</span></span></span></span> (360 kpc) projected distance to the cluster centre, which is 2–4 times larger than the spatial extent of the presently detectable X-ray-emitting intracluster medium (ICM). The mass of the Faraday-active plasma is larger than that of the X-ray-emitting ICM and exists in a density regime that broadly matches expectations for moderately dense components of the Warm-Hot Intergalactic Medium. We argue that forthcoming RM grids from both targeted and survey observations may be a singular probe of cosmic plasma in this regime. The morphology of the global Faraday depth enhancement is not uniform and isotropic but rather exhibits the classic morphology of an astrophysical bow shock on the southwest side of the main Fornax cluster, and an extended, swept-back wake on the northeastern side. Our favoured explanation for these phenomena is an ongoing merger between the main cluster and a subcluster to the southwest. The shock’s Mach angle and stand-off distance lead to a self-consistent transonic merger speed with Mach 1.06. The region hosting the Faraday depth enhancement also appears to show a decrement in both total and polarised radio emission compared to the broader field. We evaluate cosmic variance and free-free absorption by a pervasive cold dense gas surrounding NGC 1399 as possible causes but find both explanations unsatisfactory, warranting further observations. Generally, our study illustrates the scientific returns that can be expected from all-sky grids of discrete sources generated by forthcoming all-sky radio surveys.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.4" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.4" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="DF98906BA428AB755AA515F3AB1DE8A3" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"DF98906BA428AB755AA515F3AB1DE8A3","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="DF98906BA428AB755AA515F3AB1DE8A3" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="2853669" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/radio-continuum-surveys-with-square-kilometre-array-pathfinders/DF98906BA428AB755AA515F3AB1DE8A3"> Radio Continuum Surveys with Square Kilometre Array Pathfinders </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> <li><a href="/core/product/identifier/SQUARE_KILOMETRE_ARRAY/type/BESPOKE_COLLECTION" class="">Square Kilometre Array</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Ray P. 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Smith</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Grazia Umana&eventCode=SE-AU" class="more-by-this-author ">Grazia Umana</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=G.-B. Zhao&eventCode=SE-AU" class="more-by-this-author ">G.-B. Zhao</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Peter-Christian Zinn&eventCode=SE-AU" class="more-by-this-author ">Peter-Christian Zinn</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/DF38508038A251E724869CA9F573BAD5" class="productParent" data-prod-id="DF38508038A251E724869CA9F573BAD5">Volume 30</a> / 2013 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 27 March 2013</span><span class="pages">, e020</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-DF98906BA428AB755AA515F3AB1DE8A3" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/DF98906BA428AB755AA515F3AB1DE8A3/S1323358012000203a.pdf/radio_continuum_surveys_with_square_kilometre_array_pathfinders.pdf" data-pdf-content-id="DF98906BA428AB755AA515F3AB1DE8A3" target="_blank" aria-label="Download PDF for Radio Continuum Surveys with Square Kilometre Array Pathfinders [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/DF98906BA428AB755AA515F3AB1DE8A3/core-reader" target="_blank" aria-label="View HTML full text for Radio Continuum Surveys with Square Kilometre Array Pathfinders [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"DF98906BA428AB755AA515F3AB1DE8A3","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="DF98906BA428AB755AA515F3AB1DE8A3" data-container="representation" aria-label="Export citation for Radio Continuum Surveys with Square Kilometre Array Pathfinders">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pas.2012.020" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358012000203')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Radio Continuum Surveys with Square Kilometre Array Pathfinders" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"DF98906BA428AB755AA515F3AB1DE8A3"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358012000203" class="content"> <div class="abstract" data-abstract-type="normal"><p>In the lead-up to the Square Kilometre Array (SKA) project, several next-generation radio telescopes and upgrades are already being built around the world. These include APERTIF (The Netherlands), ASKAP (Australia), <span class='italic'>e</span>-MERLIN (UK), VLA (USA), e-EVN (based in Europe), LOFAR (The Netherlands), MeerKAT (South Africa), and the Murchison Widefield Array. Each of these new instruments has different strengths, and coordination of surveys between them can help maximise the science from each of them. A radio continuum survey is being planned on each of them with the primary science objective of understanding the formation and evolution of galaxies over cosmic time, and the cosmological parameters and large-scale structures which drive it. In pursuit of this objective, the different teams are developing a variety of new techniques, and refining existing ones. To achieve these exciting scientific goals, many technical challenges must be addressed by the survey instruments. Given the limited resources of the global radio-astronomical community, it is essential that we pool our skills and knowledge. We do not have sufficient resources to enjoy the luxury of re-inventing wheels. We face significant challenges in calibration, imaging, source extraction and measurement, classification and cross-identification, redshift determination, stacking, and data-intensive research. As these instruments extend the observational parameters, we will face further unexpected challenges in calibration, imaging, and interpretation. If we are to realise the full scientific potential of these expensive instruments, it is essential that we devote enough resources and careful study to understanding the instrumental effects and how they will affect the data. We have established an SKA Radio Continuum Survey working group, whose prime role is to maximise science from these instruments by ensuring we share resources and expertise across the projects. Here we describe these projects, their science goals, and the technical challenges which are being addressed to maximise the science return.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pas.2012.020" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pas.2012.020" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="051B25440FAD9218B6061DFD585B588D" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"051B25440FAD9218B6061DFD585B588D","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="051B25440FAD9218B6061DFD585B588D" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="2131400" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/askap-commissioning-observations-of-the-gama-23-field/051B25440FAD9218B6061DFD585B588D"> ASKAP commissioning observations of the GAMA 23 field </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Denis A. Leahy&eventCode=SE-AU" class="more-by-this-author ">Denis A. Leahy</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=A. M. Hopkins&eventCode=SE-AU" class="more-by-this-author ">A. M. Hopkins</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=R. P. Norris&eventCode=SE-AU" class="more-by-this-author ">R. P. Norris</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=J. Marvil&eventCode=SE-AU" class="more-by-this-author ">J. Marvil</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=J. D. Collier&eventCode=SE-AU" class="more-by-this-author ">J. D. Collier</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=E. N. Taylor&eventCode=SE-AU" class="more-by-this-author ">E. N. Taylor</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=J. R. Allison&eventCode=SE-AU" class="more-by-this-author ">J. R. 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Brown</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=S. Driver&eventCode=SE-AU" class="more-by-this-author ">S. Driver</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=G. Gurkan&eventCode=SE-AU" class="more-by-this-author ">G. Gurkan</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=L. Harvey-Smith&eventCode=SE-AU" class="more-by-this-author ">L. Harvey-Smith</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=I. Heywood&eventCode=SE-AU" class="more-by-this-author ">I. Heywood</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=B. W. Holwerda&eventCode=SE-AU" class="more-by-this-author ">B. W. Holwerda</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=J. Liske&eventCode=SE-AU" class="more-by-this-author ">J. 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Wang</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/34B96B18BAB507B4E9AF957D9C95654C" class="productParent" data-prod-id="34B96B18BAB507B4E9AF957D9C95654C">Volume 36</a> / 2019 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 19 July 2019</span><span class="pages">, e024</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-051B25440FAD9218B6061DFD585B588D" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/051B25440FAD9218B6061DFD585B588D/S132335801900016Xa.pdf/askap_commissioning_observations_of_the_gama_23_field.pdf" data-pdf-content-id="051B25440FAD9218B6061DFD585B588D" target="_blank" aria-label="Download PDF for ASKAP commissioning observations of the GAMA 23 field [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/051B25440FAD9218B6061DFD585B588D/core-reader" target="_blank" aria-label="View HTML full text for ASKAP commissioning observations of the GAMA 23 field [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"051B25440FAD9218B6061DFD585B588D","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="051B25440FAD9218B6061DFD585B588D" data-container="representation" aria-label="Export citation for ASKAP commissioning observations of the GAMA 23 field">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2019.16" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS132335801900016X')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for ASKAP commissioning observations of the GAMA 23 field" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"051B25440FAD9218B6061DFD585B588D"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS132335801900016X" class="content"> <div class="abstract" data-abstract-type="normal"><p>We have observed the G23 field of the Galaxy AndMass Assembly (GAMA) survey using the Australian Square Kilometre Array Pathfinder (ASKAP) in its commissioning phase to validate the performance of the telescope and to characterise the detected galaxy populations. This observation covers ~48 deg<span class='sup'>2</span> with synthesised beam of 32.7 arcsec by 17.8 arcsec at 936MHz, and ~39 deg<span class='sup'>2</span> with synthesised beam of 15.8 arcsec by 12.0 arcsec at 1320MHz. At both frequencies, the root-mean-square (r.m.s.) noise is ~0.1 mJy/beam. We combine these radio observations with the GAMA galaxy data, which includes spectroscopy of galaxies that are i-band selected with a magnitude limit of 19.2. Wide-field Infrared Survey Explorer (WISE) infrared (IR) photometry is used to determine which galaxies host an active galactic nucleus (AGN). In properties including source counts, mass distributions, and IR versus radio luminosity relation, the ASKAP-detected radio sources behave as expected. Radio galaxies have higher stellar mass and luminosity in IR, optical, and UV than other galaxies. We apply optical and IR AGN diagnostics and find that they disagree for ~30% of the galaxies in our sample. We suggest possible causes for the disagreement. Some cases can be explained by optical extinction of the AGN, but for more than half of the cases we do not find a clear explanation. Radio sources aremore likely (~6%) to have an AGN than radio quiet galaxies (~1%), but the majority of AGN are not detected in radio at this sensitivity.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2019.16" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2019.16" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="98E217559CC8126423FF7275790B27C0" data-mathjax-disabled="false"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"98E217559CC8126423FF7275790B27C0","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="98E217559CC8126423FF7275790B27C0" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="259" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/mwa-and-askap-observations-of-atypical-radiohalohosting-galaxy-clusters-abell-141-and-abell-3404/98E217559CC8126423FF7275790B27C0"> MWA and ASKAP observations of atypical radio-halo-hosting galaxy clusters: Abell 141 and Abell 3404 </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> <li><a href="/core/product/identifier/DE297729-82B2-4EAF-A1E8-1150AB51579E/type/BESPOKE_COLLECTION" class="">Murchison Widefield Array</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=S. W. Duchesne&eventCode=SE-AU" class="more-by-this-author ">S. W. Duchesne</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=M. Johnston-Hollitt&eventCode=SE-AU" class="more-by-this-author ">M. Johnston-Hollitt</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=A. G. Wilber&eventCode=SE-AU" class="more-by-this-author ">A. G. Wilber</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/08A6F1C86EBBD90385E0EF1AF9272071" class="productParent" data-prod-id="08A6F1C86EBBD90385E0EF1AF9272071">Volume 38</a> / 2021 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 05 July 2021</span><span class="pages">, e031</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-98E217559CC8126423FF7275790B27C0" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/98E217559CC8126423FF7275790B27C0/S1323358021000242a.pdf/mwa_and_askap_observations_of_atypical_radiohalohosting_galaxy_clusters_abell_141_and_abell_3404.pdf" data-pdf-content-id="98E217559CC8126423FF7275790B27C0" target="_blank" aria-label="Download PDF for MWA and ASKAP observations of atypical radio-halo-hosting galaxy clusters: Abell 141 and Abell 3404 [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/98E217559CC8126423FF7275790B27C0/core-reader" target="_blank" aria-label="View HTML full text for MWA and ASKAP observations of atypical radio-halo-hosting galaxy clusters: Abell 141 and Abell 3404 [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"98E217559CC8126423FF7275790B27C0","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="98E217559CC8126423FF7275790B27C0" data-container="representation" aria-label="Export citation for MWA and ASKAP observations of atypical radio-halo-hosting galaxy clusters: Abell 141 and Abell 3404">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2021.24" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358021000242')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for MWA and ASKAP observations of atypical radio-halo-hosting galaxy clusters: Abell 141 and Abell 3404" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"98E217559CC8126423FF7275790B27C0"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358021000242" class="content"> <div class="abstract" data-abstract-type="normal"><p>We report on the detection of a giant radio halo in the cluster Abell 3404 as well as confirmation of the radio halo observed in Abell 141 (with linear extents <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210702172040171-0219:S1323358021000242:S1323358021000242_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\sim\!770$</span></span></span></span> and <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210702172040171-0219:S1323358021000242:S1323358021000242_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\sim\!850$</span></span></span></span> kpc, respectively). We use the Murchison Widefield Array, the Australian Square Kilometre Array Pathfinder, and the Australia Telescope Compact Array to characterise the emission and intervening radio sources from <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210702172040171-0219:S1323358021000242:S1323358021000242_inline3.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\sim100$</span></span></span></span> to 1 000 MHz; power law models are fit to the spectral energy distributions with spectral indices <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210702172040171-0219:S1323358021000242:S1323358021000242_inline4.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\alpha_{88}^{1\,110} = -1.66 \pm 0.07$</span></span></span></span> and <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210702172040171-0219:S1323358021000242:S1323358021000242_inline5.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\alpha_{88}^{943} = -1.06 \pm 0.09$</span></span></span></span> for the radio halos in Abell 3404 and Abell 141, respectively. We find strong correlation between radio and X-ray surface brightness for Abell 3404 but little correlation for Abell 141. We note that each cluster has an atypical morphology for a radio-halo-hosting cluster, with Abell 141 having been previously reported to be in a pre-merging state, and Abell 3404 is largely relaxed with only minor evidence for a disturbed morphology. We find that the radio halo powers are consistent with the current radio halo sample and <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210702172040171-0219:S1323358021000242:S1323358021000242_inline6.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$P_\nu$</span></span></span></span>–<span class='italic'>M</span> scaling relations, but note that the radio halo in Abell 3404 is an ultra-steep–spectrum radio halo (USSRH) and, as with other USSRHs lies slightly below the best-fit <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210702172040171-0219:S1323358021000242:S1323358021000242_inline7.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$P_{1.4}$</span></span></span></span>–<span class='italic'>M</span> relation. We find that an updated scaling relation is consistent with previous results and shifting the frequency to 150 MHz does not significantly alter the best-fit relations with a sample of 86 radio halos. We suggest that the USSRH halo in Abell 3404 represents the faint class of radio halos that will be found in clusters undergoing weak mergers.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.24" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.24" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="BCD8AFB3297C3082BBF7BDCD64ED9ECF" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"BCD8AFB3297C3082BBF7BDCD64ED9ECF","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="BCD8AFB3297C3082BBF7BDCD64ED9ECF" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="297" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/lower-frequency-followup-of-28-candidate-largescale-synchrotron-sources/BCD8AFB3297C3082BBF7BDCD64ED9ECF"> Low(er) frequency follow-up of 28 candidate, large-scale synchrotron sources </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> <li><a href="/core/product/identifier/DE297729-82B2-4EAF-A1E8-1150AB51579E/type/BESPOKE_COLLECTION" class="">Murchison Widefield Array</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Torrance Hodgson&eventCode=SE-AU" class="more-by-this-author ">Torrance Hodgson</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Melanie Johnston-Hollitt&eventCode=SE-AU" class="more-by-this-author ">Melanie Johnston-Hollitt</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Benjamin McKinley&eventCode=SE-AU" class="more-by-this-author ">Benjamin McKinley</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Tessa Vernstrom&eventCode=SE-AU" class="more-by-this-author ">Tessa Vernstrom</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Valentina Vacca&eventCode=SE-AU" class="more-by-this-author ">Valentina Vacca</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/BBB6B9B8249FA0276CE235D2CE933935" class="productParent" data-prod-id="BBB6B9B8249FA0276CE235D2CE933935">Volume 37</a> / 2020 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 20 August 2020</span><span class="pages">, e032</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-BCD8AFB3297C3082BBF7BDCD64ED9ECF" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/BCD8AFB3297C3082BBF7BDCD64ED9ECF/S1323358020000260a.pdf/lower_frequency_followup_of_28_candidate_largescale_synchrotron_sources.pdf" data-pdf-content-id="BCD8AFB3297C3082BBF7BDCD64ED9ECF" target="_blank" aria-label="Download PDF for Low(er) frequency follow-up of 28 candidate, large-scale synchrotron sources [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/BCD8AFB3297C3082BBF7BDCD64ED9ECF/core-reader" target="_blank" aria-label="View HTML full text for Low(er) frequency follow-up of 28 candidate, large-scale synchrotron sources [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"BCD8AFB3297C3082BBF7BDCD64ED9ECF","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="BCD8AFB3297C3082BBF7BDCD64ED9ECF" data-container="representation" aria-label="Export citation for Low(er) frequency follow-up of 28 candidate, large-scale synchrotron sources">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2020.26" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358020000260')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Low(er) frequency follow-up of 28 candidate, large-scale synchrotron sources" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"BCD8AFB3297C3082BBF7BDCD64ED9ECF"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358020000260" class="content"> <div class="abstract" data-abstract-type="normal"><p>We follow up on a report by Vacca et al. (<a href='#r28'>2018</a>) of 28 candidate large-scale diffuse synchrotron sources in an 8<span class='sup'>°</span> × 8<span class='sup'>°</span> area of the sky (centred at RA 5<span class='sup'>h</span>0<span class='sup'>m</span>0<span class='sup'>s</span>; Dec 5<span class='sup'>°</span>48<span class='italic'>ʹ</span>00<span class='italic'>ʹʹ</span>). These sources were originally observed at 1.4 GHz using a combination of the single-dish Sardinia Radio Telescope and archival NRAO VLA Sky Survey data. They are in an area with nine massive galaxy clusters at <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20200819102137872-0360:S1323358020000260:S1323358020000260_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $z \approx 0.1$ </span></span></span></span> and are candidates for the first detection of filaments of the synchrotron cosmic web. We attempt to verify these candidate sources with lower frequency observations at 154 MHz with the Murchison Widefield Array and at 887 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP). We use a novel technique to calculate the surface brightness sensitivity of these instruments to show that our lower frequency observations, and in particular those by ASKAP, are ideally suited to detect large-scale, extended synchrotron emission. Nonetheless, we are forced to conclude that none of these sources are likely to be synchrotron in origin or associated with the cosmic web.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.26" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.26" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="A6C846F3ABB0105F026E3BD6B6EB9D19" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"A6C846F3ABB0105F026E3BD6B6EB9D19","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="A6C846F3ABB0105F026E3BD6B6EB9D19" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="2193619" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/askapemu-source-finding-data-challenge/A6C846F3ABB0105F026E3BD6B6EB9D19"> The ASKAP/EMU Source Finding Data Challenge </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> <li><a href="/core/product/identifier/127A4BF8-763B-4AB0-A0BE-BB67B2062737/type/BESPOKE_COLLECTION" class="">Data Analysis Pipelines and Software</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=A. 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Breton</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=D. Carbone&eventCode=SE-AU" class="more-by-this-author ">D. Carbone</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=C. Ferrari&eventCode=SE-AU" class="more-by-this-author ">C. Ferrari</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=T. M. O. Franzen&eventCode=SE-AU" class="more-by-this-author ">T. M. O. Franzen</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=H. Garsden&eventCode=SE-AU" class="more-by-this-author ">H. Garsden</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=J. González-Nuevo&eventCode=SE-AU" class="more-by-this-author ">J. González-Nuevo</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=C. A. Hales&eventCode=SE-AU" class="more-by-this-author ">C. A. Hales</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=P. J. Hancock&eventCode=SE-AU" class="more-by-this-author ">P. J. Hancock</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=G. Heald&eventCode=SE-AU" class="more-by-this-author ">G. Heald</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=D. Herranz&eventCode=SE-AU" class="more-by-this-author ">D. Herranz</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=M. Huynh&eventCode=SE-AU" class="more-by-this-author ">M. Huynh</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=R. J. Jurek&eventCode=SE-AU" class="more-by-this-author ">R. J. Jurek</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=M. López-Caniego&eventCode=SE-AU" class="more-by-this-author ">M. 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Shulevski</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=J. Swinbank&eventCode=SE-AU" class="more-by-this-author ">J. Swinbank</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=R. Taylor&eventCode=SE-AU" class="more-by-this-author ">R. Taylor</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=A. J. van der Horst&eventCode=SE-AU" class="more-by-this-author ">A. J. van der Horst</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/9A9F23A7E237ADB93E76A90E4F454435" class="productParent" data-prod-id="9A9F23A7E237ADB93E76A90E4F454435">Volume 32</a> / 2015 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 19 October 2015</span><span class="pages">, e037</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-A6C846F3ABB0105F026E3BD6B6EB9D19" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/A6C846F3ABB0105F026E3BD6B6EB9D19/S1323358015000375a.pdf/askapemu_source_finding_data_challenge.pdf" data-pdf-content-id="A6C846F3ABB0105F026E3BD6B6EB9D19" target="_blank" aria-label="Download PDF for The ASKAP/EMU Source Finding Data Challenge [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/A6C846F3ABB0105F026E3BD6B6EB9D19/core-reader" target="_blank" aria-label="View HTML full text for The ASKAP/EMU Source Finding Data Challenge [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"A6C846F3ABB0105F026E3BD6B6EB9D19","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="A6C846F3ABB0105F026E3BD6B6EB9D19" data-container="representation" aria-label="Export citation for The ASKAP/EMU Source Finding Data Challenge">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2015.37" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358015000375')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for The ASKAP/EMU Source Finding Data Challenge" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"A6C846F3ABB0105F026E3BD6B6EB9D19"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358015000375" class="content"> <div class="abstract" data-abstract-type="normal"><p>The Evolutionary Map of the Universe (EMU) is a proposed radio continuum surveyof the Southern Hemisphere up to declination + 30°, with the AustralianSquare Kilometre Array Pathfinder (ASKAP). EMU will use an automated sourceidentification and measurement approach that is demonstrably optimal, tomaximise the reliability and robustness of the resulting radio sourcecatalogues. As a step toward this goal we conducted a “DataChallenge” to test a variety of source finders on simulated images. Theaim is to quantify the accuracy and limitations of existing automated sourcefinding and measurement approaches. The Challenge initiators also tested thecurrent ASKAPsoft source-finding tool to establish how it could benefit fromincorporating successful features of the other tools. As expected, most findersshow completeness around 100% at ≈ 10σ dropping to about 10% by≈ 5σ. Reliability is typically close to 100% at ≈10σ, with performance to lower sensitivities varying between finders. Allfinders show the expected trade-off, where a high completeness at lowsignal-to-noise gives a corresponding reduction in reliability, and vice versa.We conclude with a series of recommendations for improving the performance ofthe ASKAPsoft source-finding tool.</p> </div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2015.37" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2015.37" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="F13448BAE494998F59942A4C9F1EED58" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"F13448BAE494998F59942A4C9F1EED58","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="F13448BAE494998F59942A4C9F1EED58" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="184" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/askap-reveals-giant-radio-halos-in-two-merging-spt-galaxy-clusters/F13448BAE494998F59942A4C9F1EED58"> ASKAP reveals giant radio halos in two merging SPT galaxy clusters </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Amanda G. Wilber&eventCode=SE-AU" class="more-by-this-author ">Amanda G. Wilber</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Melanie Johnston-Hollitt&eventCode=SE-AU" class="more-by-this-author ">Melanie Johnston-Hollitt</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Stefan W. Duchesne&eventCode=SE-AU" class="more-by-this-author ">Stefan W. Duchesne</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Cyril Tasse&eventCode=SE-AU" class="more-by-this-author ">Cyril Tasse</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Hiroki Akamatsu&eventCode=SE-AU" class="more-by-this-author ">Hiroki Akamatsu</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Huib Intema&eventCode=SE-AU" class="more-by-this-author ">Huib Intema</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Torrance Hodgson&eventCode=SE-AU" class="more-by-this-author ">Torrance Hodgson</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/BBB6B9B8249FA0276CE235D2CE933935" class="productParent" data-prod-id="BBB6B9B8249FA0276CE235D2CE933935">Volume 37</a> / 2020 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 08 October 2020</span><span class="pages">, e040</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-F13448BAE494998F59942A4C9F1EED58" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/F13448BAE494998F59942A4C9F1EED58/S132335802000034Xa.pdf/askap_reveals_giant_radio_halos_in_two_merging_spt_galaxy_clusters.pdf" data-pdf-content-id="F13448BAE494998F59942A4C9F1EED58" target="_blank" aria-label="Download PDF for ASKAP reveals giant radio halos in two merging SPT galaxy clusters [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/F13448BAE494998F59942A4C9F1EED58/core-reader" target="_blank" aria-label="View HTML full text for ASKAP reveals giant radio halos in two merging SPT galaxy clusters [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"F13448BAE494998F59942A4C9F1EED58","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="F13448BAE494998F59942A4C9F1EED58" data-container="representation" aria-label="Export citation for ASKAP reveals giant radio halos in two merging SPT galaxy clusters">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2020.34" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS132335802000034X')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for ASKAP reveals giant radio halos in two merging SPT galaxy clusters" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"F13448BAE494998F59942A4C9F1EED58"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS132335802000034X" class="content"> <div class="abstract" data-abstract-type="normal"><p>Early science observations from the Australian Square Kilometre Array Pathfinder (ASKAP) have revealed clear signals of diffuse radio emission associated with two clusters detected by the South Pole Telescope via their Sunyaev Zel’dovich signal: SPT CLJ0553-3342 (MACS J0553.4-3342) and SPT CLJ0638-5358 (Abell S0592) are both high-mass lensing clusters that have undergone major mergers. To create science-fidelity images of the galaxy clusters, we performed direction-dependent (DD) calibration and imaging on these ASKAP early science observations using state-of-the-art software killMS and DDFacet. Here, we present our DD calibrated ASKAP radio images of both clusters showing unambiguous giant radio halos with largest linear scales of <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201007123744291-0294:S132335802000034X:S132335802000034X_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> ${\sim}1$ </span></span></span></span> Mpc. The halo in MACS J0553.4-3342 was previously detected with Giant Metrewave Radio Telescope observations at 323 MHz but appears more extended in our ASKAP image. Although there is a shock detected in the thermal X-ray emission of this cluster, we find that the particle number density in the shocked region is too low to allow for the generation of a radio shock. The radio halo in Abell S0592 is a new discovery, and the Southwest border of the halo coincides with a shock detected in X-rays. We discuss the origins of these halos considering both the hadronic and turbulent re-acceleration models and sources of <span class='italic'>seed</span> electrons. This work gives a positive indication of the potential of ASKAP’s Evolutionary Map of the Universe survey in detecting intracluster medium radio sources.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.34" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.34" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="A933216C043401066969100E10139614" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"A933216C043401066969100E10139614","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="A933216C043401066969100E10139614" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="1858969" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/australian-square-kilometre-array-pathfinder-performance-of-the-boolardy-engineering-test-array/A933216C043401066969100E10139614"> The Australian Square Kilometre Array Pathfinder: Performance of the Boolardy Engineering Test Array </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=D. 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Boolardy Engineering Test Array is the first aperture synthesis radio telescope to use phased array feed technology, giving it the ability to electronically form up to nine dual-polarisation beams. We report the methods developed for forming and measuring the beams, and the adaptations that have been made to the traditional calibration and imaging procedures in order to allow BETA to function as a multi-beam aperture synthesis telescope. We describe the commissioning of the instrument and present details of Boolardy Engineering Test Array’s performance: sensitivity, beam characteristics, polarimetric properties, and image quality. We summarise the astronomical science that it has produced and draw lessons from operating Boolardy Engineering Test Array that will be relevant to the commissioning and operation of the final Australian Square Kilometre Array Path telescope.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2016.37" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2016.37" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="6FD673731F193C01A133A89602B75F86" data-mathjax-disabled="false"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"6FD673731F193C01A133A89602B75F86","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="6FD673731F193C01A133A89602B75F86" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="411" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/evolutionary-map-of-the-universe-pilot-survey/6FD673731F193C01A133A89602B75F86"> The Evolutionary Map of the Universe pilot survey </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Ray P. 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if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="6FD673731F193C01A133A89602B75F86" data-container="representation" aria-label="Export citation for The Evolutionary Map of the Universe pilot survey">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2021.42" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358021000424')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for The Evolutionary Map of the Universe pilot survey" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"6FD673731F193C01A133A89602B75F86"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358021000424" class="content"> <div class="abstract" data-abstract-type="normal"> <p>We present the data and initial results from the first pilot survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The survey covers <span class='inlineFormula'> <span class='alternatives'> <img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210906095204165-0100:S1323358021000424:S1323358021000424_inline1.png'> <span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $270 \,\mathrm{deg}^2$ </span></span> </span> </span> of an area covered by the Dark Energy Survey, reaching a depth of 25–30 <span class='inlineFormula'> <span class='alternatives'> <img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210906095204165-0100:S1323358021000424:S1323358021000424_inline2.png'> <span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\mu\mathrm{Jy\ beam}^{-1}$ </span></span> </span> </span> rms at a spatial resolution of <span class='inlineFormula'> <span class='alternatives'> <img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210906095204165-0100:S1323358021000424:S1323358021000424_inline3.png'> <span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\sim$ </span></span> </span> </span>11–18 arcsec, resulting in a catalogue of <span class='inlineFormula'> <span class='alternatives'> <img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210906095204165-0100:S1323358021000424:S1323358021000424_inline4.png'> <span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\sim$ </span></span> </span> </span>220 000 sources, of which <span class='inlineFormula'> <span class='alternatives'> <img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210906095204165-0100:S1323358021000424:S1323358021000424_inline5.png'> <span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\sim$ </span></span> </span> </span>180 000 are single-component sources. Here we present the catalogue of single-component sources, together with (where available) optical and infrared cross-identifications, classifications, and redshifts. This survey explores a new region of parameter space compared to previous surveys. Specifically, the EMU Pilot Survey has a high density of sources, and also a high sensitivity to low surface brightness emission. These properties result in the detection of types of sources that were rarely seen in or absent from previous surveys. We present some of these new results here.</p> </div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.42" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.42" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="CEFDF9239B2DC09A194FE66F52846C8C" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"CEFDF9239B2DC09A194FE66F52846C8C","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="CEFDF9239B2DC09A194FE66F52846C8C" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="143" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/rapid-askap-continuum-survey-i-design-and-first-results/CEFDF9239B2DC09A194FE66F52846C8C"> The Rapid ASKAP Continuum Survey I: Design and first results </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=D. 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Voronkov</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Tobias Westmeier&eventCode=SE-AU" class="more-by-this-author ">Tobias Westmeier</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/BBB6B9B8249FA0276CE235D2CE933935" class="productParent" data-prod-id="BBB6B9B8249FA0276CE235D2CE933935">Volume 37</a> / 2020 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 30 November 2020</span><span class="pages">, e048</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-CEFDF9239B2DC09A194FE66F52846C8C" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/CEFDF9239B2DC09A194FE66F52846C8C/S1323358020000417a.pdf/rapid_askap_continuum_survey_i_design_and_first_results.pdf" data-pdf-content-id="CEFDF9239B2DC09A194FE66F52846C8C" target="_blank" aria-label="Download PDF for The Rapid ASKAP Continuum Survey I: Design and first results [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/CEFDF9239B2DC09A194FE66F52846C8C/core-reader" target="_blank" aria-label="View HTML full text for The Rapid ASKAP Continuum Survey I: Design and first results [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"CEFDF9239B2DC09A194FE66F52846C8C","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="CEFDF9239B2DC09A194FE66F52846C8C" data-container="representation" aria-label="Export citation for The Rapid ASKAP Continuum Survey I: Design and first results">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2020.41" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358020000417')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for The Rapid ASKAP Continuum Survey I: Design and first results" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"CEFDF9239B2DC09A194FE66F52846C8C"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358020000417" class="content"> <div class="abstract" data-abstract-type="normal"><p>The Rapid ASKAP Continuum Survey (RACS) is the first large-area survey to be conducted with the full 36-antenna Australian Square Kilometre Array Pathfinder (ASKAP) telescope. RACS will provide a shallow model of the ASKAP sky that will aid the calibration of future deep ASKAP surveys. RACS will cover the whole sky visible from the ASKAP site in Western Australia and will cover the full ASKAP band of 700–1800 MHz. The RACS images are generally deeper than the existing NRAO VLA Sky Survey and Sydney University Molonglo Sky Survey radio surveys and have better spatial resolution. All RACS survey products will be public, including radio images (with <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201127070547674-0824:S1323358020000417:S1323358020000417_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\sim$ </span></span></span></span> 15 arcsec resolution) and catalogues of about three million source components with spectral index and polarisation information. In this paper, we present a description of the RACS survey and the first data release of 903 images covering the sky south of declination <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201127070547674-0824:S1323358020000417:S1323358020000417_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $+41^\circ$ </span></span></span></span> made over a 288-MHz band centred at 887.5 MHz.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.41" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.41" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="62FE0D4D1D5A96A592A866EA296C62F6" data-mathjax-disabled="false"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"62FE0D4D1D5A96A592A866EA296C62F6","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="62FE0D4D1D5A96A592A866EA296C62F6" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="251" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/astrometric-accuracy-of-snapshot-fast-radio-burst-localisations-with-askap/62FE0D4D1D5A96A592A866EA296C62F6"> Astrometric accuracy of snapshot fast radio burst localisations with ASKAP </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Cherie K. Day&eventCode=SE-AU" class="more-by-this-author ">Cherie K. Day</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Adam T. Deller&eventCode=SE-AU" class="more-by-this-author ">Adam T. Deller</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Clancy W. James&eventCode=SE-AU" class="more-by-this-author ">Clancy W. James</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Emil Lenc&eventCode=SE-AU" class="more-by-this-author ">Emil Lenc</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Shivani Bhandari&eventCode=SE-AU" class="more-by-this-author ">Shivani Bhandari</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=R. M. Shannon&eventCode=SE-AU" class="more-by-this-author ">R. M. Shannon</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Keith W. Bannister&eventCode=SE-AU" class="more-by-this-author ">Keith W. Bannister</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/08A6F1C86EBBD90385E0EF1AF9272071" class="productParent" data-prod-id="08A6F1C86EBBD90385E0EF1AF9272071">Volume 38</a> / 2021 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 21 September 2021</span><span class="pages">, e050</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-62FE0D4D1D5A96A592A866EA296C62F6" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/62FE0D4D1D5A96A592A866EA296C62F6/S1323358021000400a.pdf/astrometric_accuracy_of_snapshot_fast_radio_burst_localisations_with_askap.pdf" data-pdf-content-id="62FE0D4D1D5A96A592A866EA296C62F6" target="_blank" aria-label="Download PDF for Astrometric accuracy of snapshot fast radio burst localisations with ASKAP [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/62FE0D4D1D5A96A592A866EA296C62F6/core-reader" target="_blank" aria-label="View HTML full text for Astrometric accuracy of snapshot fast radio burst localisations with ASKAP [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"62FE0D4D1D5A96A592A866EA296C62F6","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="62FE0D4D1D5A96A592A866EA296C62F6" data-container="representation" aria-label="Export citation for Astrometric accuracy of snapshot fast radio burst localisations with ASKAP">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2021.40" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358021000400')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Astrometric accuracy of snapshot fast radio burst localisations with ASKAP" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"62FE0D4D1D5A96A592A866EA296C62F6"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358021000400" class="content"> <div class="abstract" data-abstract-type="normal"><p>The recent increase in well-localised fast radio bursts (FRBs) has facilitated in-depth studies of global FRB host properties, the source circumburst medium, and the potential impacts of these environments on the burst properties. The Australian Square Kilometre Array Pathfinder (ASKAP) has localised 11 FRBs with sub-arcsecond to arcsecond precision, leading to sub-galaxy localisation regions in some cases and those covering much of the host galaxy in others. The method used to astrometrically register the FRB image frame for ASKAP, in order to align it with images taken at other wavelengths, is currently limited by the brightness of continuum sources detected in the short-duration (‘snapshot’) voltage data captured by the Commensal Real-Time ASKAP Fast Transients (CRAFT) software correlator, which are used to correct for any frame offsets due to imperfect calibration solutions and estimate the accuracy of any required correction. In this paper, we use dedicated observations of bright, compact radio sources in the low- and mid-frequency bands observable by ASKAP to investigate the typical astrometric accuracy of the positions obtained using this so-called ‘snapshot’ technique. Having captured these data with both the CRAFT software and ASKAP hardware correlators, we also compare the offset distributions obtained from both data products to estimate a typical offset between the image frames resulting from the differing processing paths, laying the groundwork for future use of the longer duration, higher signal-to-noise ratio (S/N) data recorded by the hardware correlator. We find typical offsets between the two frames of <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210920092824963-0975:S1323358021000400:S1323358021000400_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> ${\sim}0.6$ </span></span></span></span> and <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20210920092824963-0975:S1323358021000400:S1323358021000400_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> ${\sim}0.3$ </span></span></span></span> arcsec in the low- and mid-band data, respectively, for both RA and Dec. We also find reasonable agreement between our offset distributions and those of the published FRBs. We detect only a weak dependence in positional offset on the relative separation in time and elevation between target and calibrator scans, with the trends being more pronounced in the low-band data and in Dec. Conversely, the offsets show a clear dependence on frequency in the low band, which we compare to the frequency-dependent Dec. offsets found in FRB 200430. In addition, we present a refined methodology for estimating the overall astrometric accuracy of CRAFT FRBs.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.40" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.40" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="1BBB709579955CD5DCD8E029F80D48B1" data-mathjax-disabled="true"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"1BBB709579955CD5DCD8E029F80D48B1","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="1BBB709579955CD5DCD8E029F80D48B1" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="254" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/capability-of-the-australian-square-kilometre-array-pathfinder-to-detect-prompt-radio-bursts-from-neutron-star-mergers/1BBB709579955CD5DCD8E029F80D48B1"> The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> <li><a href="/core/product/identifier/B68A5E8B-5504-4505-828F-5314DA5EC589/type/BESPOKE_COLLECTION" class="">Gravitational Wave Astronomy</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=Ziteng Wang&eventCode=SE-AU" class="more-by-this-author ">Ziteng Wang</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Tara Murphy&eventCode=SE-AU" class="more-by-this-author ">Tara Murphy</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=David L. Kaplan&eventCode=SE-AU" class="more-by-this-author ">David L. Kaplan</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Keith W. Bannister&eventCode=SE-AU" class="more-by-this-author ">Keith W. Bannister</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=Dougal Dobie&eventCode=SE-AU" class="more-by-this-author ">Dougal Dobie</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/BBB6B9B8249FA0276CE235D2CE933935" class="productParent" data-prod-id="BBB6B9B8249FA0276CE235D2CE933935">Volume 37</a> / 2020 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 02 December 2020</span><span class="pages">, e051</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-1BBB709579955CD5DCD8E029F80D48B1" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/1BBB709579955CD5DCD8E029F80D48B1/S1323358020000429a.pdf/capability_of_the_australian_square_kilometre_array_pathfinder_to_detect_prompt_radio_bursts_from_neutron_star_mergers.pdf" data-pdf-content-id="1BBB709579955CD5DCD8E029F80D48B1" target="_blank" aria-label="Download PDF for The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/1BBB709579955CD5DCD8E029F80D48B1/core-reader" target="_blank" aria-label="View HTML full text for The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"1BBB709579955CD5DCD8E029F80D48B1","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="1BBB709579955CD5DCD8E029F80D48B1" data-container="representation" aria-label="Export citation for The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2020.42" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS1323358020000429')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"1BBB709579955CD5DCD8E029F80D48B1"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS1323358020000429" class="content"> <div class="abstract" data-abstract-type="normal"><p>We discuss observational strategies to detect prompt bursts associated with gravitational wave (GW) events using the Australian Square Kilometre Array Pathfinder (ASKAP). Many theoretical models of binary neutron stars mergers predict that bright, prompt radio emission would accompany the merger. The detection of such prompt emission would greatly improve our knowledge of the physical conditions, environment, and location of the merger. However, searches for prompt emission are complicated by the relatively poor localisation for GW events, with the 90% credible region reaching hundreds or even thousands of square degrees. Operating in fly’s eye mode, the ASKAP field of view can reach <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201201173206353-0611:S1323358020000429:S1323358020000429_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\sim1\,000$</span></span></span></span> deg<span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201201173206353-0611:S1323358020000429:S1323358020000429_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$^2$</span></span></span></span> at <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201201173206353-0611:S1323358020000429:S1323358020000429_inline3.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\sim$</span></span></span></span><span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201201173206353-0611:S1323358020000429:S1323358020000429_inline4.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$888\,{\rm MHz}$</span></span></span></span>. This potentially allows observers to cover most of the 90% credible region quickly enough to detect prompt emission. We use skymaps for GW170817 and GW190814 from LIGO/Virgo’s third observing run to simulate the probability of detecting prompt emission for GW events in the upcoming fourth observing run. With only alerts released after merger, we find it difficult to slew the telescope sufficiently quickly as to capture any prompt emission. However, with the addition of alerts released <span class='italic'>before</span> merger by negative-latency pipelines, we find that it should be possible to search for nearby, bright prompt fast radio burst-like emission from GW events. Nonetheless, the rates are low: we would expect to observe <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20201201173206353-0611:S1323358020000429:S1323358020000429_inline5.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'>$\sim$</span></span></span></span>0.012 events during the fourth observing run, assuming that the prompt emission is emitted microseconds around the merger.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.42" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2020.42" data-link-target="_blank"></div> </div> </div> </div> <div class="representation overview search" data-prod-id="3317DE9DF58A437DF223A431519C83A8" data-mathjax-disabled="false"> <div class="row"> <div class="small-1 columns checklist-col"> <label class="product-listing-with-inputs-input"> <input type="checkbox" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"3317DE9DF58A437DF223A431519C83A8","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}' name="productParts" style="display: inline-block" data-prod-id="3317DE9DF58A437DF223A431519C83A8" data-prod-source="listing" data-prod-type="JOURNAL_ARTICLE" data-file-size="258" data-has-entitlement="true" data-has-pdf="true" /> </label> </div> <div class="product-listing-with-inputs-content"> <div class="small-10 columns margin-bottom"> <ul class="details"> <li class="title"><h3><a class="part-link" href="/core/journals/publications-of-the-astronomical-society-of-australia/article/lowfrequency-integrated-radio-spectra-of-diffuse-steepspectrum-sources-in-galaxy-clusters-palaeontology-with-the-mwa-and-askap/3317DE9DF58A437DF223A431519C83A8"> Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP </a></h3></li> <li> Part of: <ul class="partOfCollection"> <li><a href="/core/product/identifier/DE297729-82B2-4EAF-A1E8-1150AB51579E/type/BESPOKE_COLLECTION" class="">Murchison Widefield Array</a></li> <li><a href="/core/product/identifier/ASKAP/type/BESPOKE_COLLECTION" class="">Australian SKA Pathfinder</a></li> </ul> </li> <li class="author"> <a href="/core/search?filters%5BauthorTerms%5D=S. W. Duchesne&eventCode=SE-AU" class="more-by-this-author ">S. W. Duchesne</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=M. Johnston-Hollitt&eventCode=SE-AU" class="more-by-this-author ">M. Johnston-Hollitt</a><span class="separator">, </span><a href="/core/search?filters%5BauthorTerms%5D=I. Bartalucci&eventCode=SE-AU" class="more-by-this-author ">I. Bartalucci</a> </li> <li> <dl> <dt class="source dl-inline">Journal: </dt> <dd> <a class="productParent" data-prod-id="EA97E060D413517C6C4433BED25DDCA9" href="/core/journals/publications-of-the-astronomical-society-of-australia">Publications of the Astronomical Society of Australia</a> / <a href="/core/product/08A6F1C86EBBD90385E0EF1AF9272071" class="productParent" data-prod-id="08A6F1C86EBBD90385E0EF1AF9272071">Volume 38</a> / 2021 </dd> <dt class="published dl-inline">Published online by Cambridge University Press: </dt> <dd> <span class="date"> 12 October 2021</span><span class="pages">, e053</span> </dd> </dl> </li> <li> <ul class="access links"> <li class="type article">Article</li> <li> <ul class="access-modal"> <li class="status entitled"> <span class="sr-only">You have access </span> <span class="entitled status-text" title="You have access to this product" aria-hidden="true">Access</span> <span class="icon access-icon cursorDefault" title="You have access to this product" aria-hidden="true"> <svg id="access-3317DE9DF58A437DF223A431519C83A8" xmlns="http://www.w3.org/2000/svg" viewBox="-701.2 242.7 206.9 328.3"> <circle class="st0" fill="#229619" cx="-597.9" cy="413.8" r="102.5"/> <path class="st1" fill="#fff" d="M-616 472.4l-49.6-49.6 26.5-26.5 23.1 23 59.3-59.3 26.5 26.5z"/> </svg> </span> </li> <li class="status open-access"> </li> </ul> </li> <li> <a href="/core/services/aop-cambridge-core/content/view/3317DE9DF58A437DF223A431519C83A8/S132335802100045Xa.pdf/lowfrequency_integrated_radio_spectra_of_diffuse_steepspectrum_sources_in_galaxy_clusters_palaeontology_with_the_mwa_and_askap.pdf" data-pdf-content-id="3317DE9DF58A437DF223A431519C83A8" target="_blank" aria-label="Download PDF for Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP [Opens in a new window]" > <span class="icon icn pdf"> <span class="download-label">PDF </span> </span> </a> </li> <li> <a href="/core/product/3317DE9DF58A437DF223A431519C83A8/core-reader" target="_blank" aria-label="View HTML full text for Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP [Opens in a new window]" data-cup-event-payload='{"eventCode":"DL-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","productId":"3317DE9DF58A437DF223A431519C83A8","referringURL":"","authenticationMethods":[],"usedIdentities":["0"],"searchScope":"PRODUCT"}'> <span class="icon icn html wide"> <span class="download-label">HTML</span> </span> </a> </li> <li> <script> $(document).ready(function () { /** * Disable tooltip aria label attributes, so the screen reader can correctly read out the core * reader tab navigation. * Set a short delay, so we can be sure the tooltips have rendered, before updating the DOM. */ setTimeout(function () { var $downloadLinks = $('.download-types li a'); if ($downloadLinks.length) { $downloadLinks.attr('role', 'tab'); $downloadLinks.attr('aria-describedby', ''); // Remove the aria alerts on the tool tips $('.qtip').attr('role', 'none'); } }, 500); }); </script> </li> <li><a href="#" class="export-citation-component" data-prod-id="3317DE9DF58A437DF223A431519C83A8" data-container="representation" aria-label="Export citation for Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP">Export citation </a></li> <li> <a href="https://ui.adsabs.harvard.edu/abs/10.1017/pasa.2021.45" class="adsabs-link" target="_blank"> NASA ADS Abstract Service </a> </li> </ul> </li> <li class="accordion no-margin-top abstract" data-accordion> <div class="accordion-navigation"> <button onclick="toggleViewHide(this, 'abstractS132335802100045X')" class="button-no-transition transparent-no-border" aria-expanded="false" aria-label="View Abstract for Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP" data-cup-event='{"eventCode":"IN-AR","eventContext":"/core/journals/publications-of-the-astronomical-society-of-australia/collections/australian-ska-pathfinder","usedIdentities":[],"authenticationMethods":[],"referringURL":"","eventType":"VADE","searchScope":"PRODUCT","productId":"3317DE9DF58A437DF223A431519C83A8"}' data-cup-event-disable-on-hide="true" > <div class="icon open-drawer small"> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 17 17" class="is-opened"> <circle fill="#696969" cx="8.5" cy="8.5" r="7.5"/> <circle fill="#FFF" cx="8.5" cy="8.5" r="7"/> <path fill="#696969" d="M12.6 7.3H4.4c-.8 0-1.4.5-1.4 1.2s.6 1.2 1.4 1.2h8.3c.8 0 1.4-.5 1.4-1.2-.1-.7-.7-1.2-1.5-1.2z"/> </svg> <svg xmlns="http://www.w3.org/2000/svg" width="15" height="15" viewBox="0 0 15 15" class="is-closed"> <g transform="translate(1 1)" fill="none" fill-rule="evenodd"> <circle fill="#696969" cx="6.5" cy="6.5" r="6.5"/> <circle fill="#FFF" cx="6.5" cy="6.5" r="6"/> <path d="M9.855 5.518H7.482V3.145C7.482 2.491 7.072 2 6.5 2c-.573 0-.982.49-.982 1.145V5.518H3.145C2.491 5.518 2 5.928 2 6.5c0 .573.49.982 1.145.982H5.518v2.372c0 .655.41 1.146.982 1.146.573 0 .982-.49.982-1.145V7.482h2.372c.655 0 1.146-.41 1.146-.982 0-.573-.49-.982-1.145-.982z" fill="#696969"/> </g> </svg> <span class="toggle-text">View </span> <span class="excerpt-type">abstract</span> </div> </button> <div id="abstractS132335802100045X" class="content"> <div class="abstract" data-abstract-type="normal"><p>Galaxy clusters have been found to host a range of diffuse, non-thermal emission components, generally with steep, power law spectra. In this work we report on the detection and follow-up of radio halos, relics, remnant radio galaxies, and other fossil radio plasmas in Southern Sky galaxy clusters using the Murchison Widefield Array and the Australian Square Kilometre Array Pathfinder. We make use of the frequency coverage between the two radio interferometers—from 88 to <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20211011101104601-0341:S132335802100045X:S132335802100045X_inline1.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\sim\!900$ </span></span></span></span> MHz—to characterise the integrated spectra of these sources within this frequency range. Highlights from the sample include the detection of a double relic system in Abell 3186, a mini-halo in RXC J0137.2–0912, a candidate halo and relic in Abell 3399, and a complex multi-episodic head-tail radio galaxy in Abell 3164. We compare this selection of sources and candidates to the literature sample, finding sources consistent with established radio power–cluster mass scaling relations. Finally, we use the low-frequency integrated spectral index, <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20211011101104601-0341:S132335802100045X:S132335802100045X_inline2.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\alpha$ </span></span></span></span> (<span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20211011101104601-0341:S132335802100045X:S132335802100045X_inline3.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $S_v \propto v^\alpha$ </span></span></span></span>), of the detected sample of cluster remnants and fossil sources to compare with samples of known halos, relics, remnants and fossils to investigate a possible link between their electron populations. We find the distributions of <span class='inlineFormula'><span class='alternatives'><img class='inline-graphic mathjax-alternative mathjax-alt-graphic mathjax-off' data-mimesubtype='png' data-type='' src='//static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20211011101104601-0341:S132335802100045X:S132335802100045X_inline4.png'><span class='mathjax-tex-wrapper' data-mathjax-type='texmath'><span class='tex-math mathjax-tex-math mathjax-on'> $\alpha$ </span></span></span></span> to be consistent with relic and halo emission generated by seed electrons that originated in fossil or remnant sources. However, the present sample sizes are insufficient to rule out other scenarios.</p></div> </div> </div> </li> </ul> </div> <div class="small-6 medium-1 large-1 right hide-for-small altmetric-embed altmetric-core-desktop" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.45" data-link-target="_blank"></div> <div class="small-6 columns right text-center hide-for-medium-up altmetric-embed altmetric-core-mobile" data-badge-type='donut' data-hide-less-than="1" data-doi="10.1017/pasa.2021.45" data-link-target="_blank"></div> </div> </div> </div> </div> </div> <hr/> <div class="pagination-centered" data-test-id="paginationSearchResult"> <p class="paragraph_05 margin-bottom-small">Page 1 of 2</p> <ul class="pagination"> <li class="unavailable"><span class="in-active-item">First</span></li> <li class="unavailable"><span class="in-active-item">« Prev</span></li> <li class="current"><a href="?pageNum=1" data-page-number="1" aria-label="Page 1">1</a></li> <li class=""><a 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