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overflow: hidden; text-overflow: ellipsis; -webkit-line-clamp: 3; -webkit-box-orient: vertical; }</style><div class="col-xs-12 clearfix"><div class="u-floatLeft"><h1 class="PageHeader-title u-m0x u-fs30">Herschel Space Observatory</h1><div class="u-tcGrayDark">30 Followers</div><div class="u-tcGrayDark u-mt2x">Recent papers in <b>Herschel Space Observatory</b></div></div></div></div></div></div><div class="TabbedNavigation"><div class="container"><div class="row"><div class="col-xs-12 clearfix"><ul class="nav u-m0x u-p0x list-inline u-displayFlex"><li class="active"><a href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Top Papers</a></li><li><a href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory/MostCited">Most Cited Papers</a></li><li><a href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory/MostDownloaded">Most Downloaded Papers</a></li><li><a href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory/MostRecent">Newest Papers</a></li><li><a class="" href="https://www.academia.edu/People/Herschel_Space_Observatory">People</a></li></ul></div><style type="text/css">ul.nav{flex-direction:row}@media(max-width: 567px){ul.nav{flex-direction:column}.TabbedNavigation li{max-width:100%}.TabbedNavigation li.active{background-color:var(--background-grey, #dddde2)}.TabbedNavigation li.active:before,.TabbedNavigation li.active:after{display:none}}</style></div></div></div><div class="container"><div class="row"><div class="col-xs-12"><div class="u-displayFlex"><div class="u-flexGrow1"><div class="works"><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_21812412" data-work_id="21812412" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/21812412/The_Photodetector_Array_Camera_and_Spectrometer_PACS_on_the_Herschel_Space_Observatory">The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/21812412" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="cc29490cfd2028c82b775de2b04093ee" rel="nofollow" data-download="{"attachment_id":42570684,"asset_id":21812412,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/42570684/download_file?st=MTczMzI2NjQ0MSw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="43036512" href="https://independent.academia.edu/JCepa1">J. 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It will survey 510 square degrees of the extragalactic sky, four times larger than all the other Herschel surveys... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_5959010" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 510 square degrees of the extragalactic sky, four times larger than all the other Herschel surveys combined, in five far-infrared and submillimetre bands. We describe the survey, the complementary multi-wavelength datasets that will be combined with the Herschel data, and the six major science programmes we are undertaking. Using new models based on a previous submillimetre survey of galaxies, we present predictions of the properties of the ATLAS sources in other wavebands.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/5959010" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="bada84cc3cacd273dbc5e23dbce8cc9e" rel="nofollow" data-download="{"attachment_id":32923304,"asset_id":5959010,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/32923304/download_file?st=MTczMzI2NjQ0MSw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="622080" href="https://leicester.academia.edu/JonathanATedds">Jonathan A. 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href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="92750" href="https://www.academia.edu/Documents/in/Noise_estimation">Noise estimation</a>, <script data-card-contents-for-ri="92750" type="text/json">{"id":92750,"name":"Noise estimation","url":"https://www.academia.edu/Documents/in/Noise_estimation?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="453368" href="https://www.academia.edu/Documents/in/Spatial_Variation">Spatial Variation</a><script data-card-contents-for-ri="453368" type="text/json">{"id":453368,"name":"Spatial 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the stolen starlight with Herschel</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/32681838" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="a15850a84545477ca1a6d66ce584a249" rel="nofollow" data-download="{"attachment_id":52847310,"asset_id":32681838,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/52847310/download_file?st=MTczMzI2NjQ0MSw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="32822" href="https://cardiff.academia.edu/EdwardGomez">Edward Gomez</a><script data-card-contents-for-user="32822" type="text/json">{"id":32822,"first_name":"Edward","last_name":"Gomez","domain_name":"cardiff","page_name":"EdwardGomez","display_name":"Edward Gomez","profile_url":"https://cardiff.academia.edu/EdwardGomez?f_ri=15306","photo":"https://0.academia-photos.com/32822/10632/102685/s65_edward.gomez.jpg"}</script></span></span></li><li class="js-paper-rank-work_32681838 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="32681838"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 32681838, container: ".js-paper-rank-work_32681838", }); });</script></li><li class="js-percentile-work_32681838 InlineList-item InlineList-item--bordered hidden u-tcGrayDark"><span class="percentile-widget hidden"><span class="u-mr2x percentile-widget" style="display: none">•</span><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 32681838; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = 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class="InlineList-item-text" data-has-card-for-ri="432026" href="https://www.academia.edu/Documents/in/Public_Interest">Public Interest</a>, <script data-card-contents-for-ri="432026" type="text/json">{"id":432026,"name":"Public Interest","url":"https://www.academia.edu/Documents/in/Public_Interest?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="911616" href="https://www.academia.edu/Documents/in/Space_Missions">Space Missions</a><script data-card-contents-for-ri="911616" type="text/json">{"id":911616,"name":"Space Missions","url":"https://www.academia.edu/Documents/in/Space_Missions?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=32681838]'), work: {"id":32681838,"title":"Seeing the stolen starlight with 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Interest","url":"https://www.academia.edu/Documents/in/Public_Interest?f_ri=15306","nofollow":false},{"id":911616,"name":"Space Missions","url":"https://www.academia.edu/Documents/in/Space_Missions?f_ri=15306","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_4440853" data-work_id="4440853" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/4440853/Herschel_SPIRE_design_performance_and_scientific_capabilities">Herschel-SPIRE: design, performance, and scientific capabilities</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">SPIRE, the Spectral and Photometric Imaging Receiver, is a submillimetre camera and spectrometer for the European Space Agency's Herschel Space Observatory. It comprises a three-band imaging photometer operating at 250, 360 and 520 μm,... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_4440853" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">SPIRE, the Spectral and Photometric Imaging Receiver, is a submillimetre camera and spectrometer for the European Space Agency's Herschel Space Observatory. It comprises a three-band imaging photometer operating at 250, 360 and 520 μm, and an imaging Fourier Transform Spectrometer (FTS) covering 200-670 μm. The detectors are arrays of feedhorn-coupled NTD spider-web bolometers cooled to 0.3 K. The photometer field of view of is 4 x 8 arcmin., observed simultaneously in the three spectral bands. The FTS has an approximately circular field of view with a diameter of 2.6 arcmin., and employs a dual-beam configuration with broad-band intensity beam dividers to provide high efficiency and separated output and input ports. The spectral resolution can be adjusted between 0.04 and 2 cm-1 (resolving power of 20-1000 at 250 μm). The flight instrument is currently undergoing integration and test. The design of SPIRE is described, and the expected scientific performance is summarised, based on modelling and flight instrument test results.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/4440853" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="db0c1e1be52bd512422b5d858187dfb4" rel="nofollow" data-download="{"attachment_id":49859171,"asset_id":4440853,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/49859171/download_file?st=MTczMzI2NjQ0MSw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="5463980" href="https://independent.academia.edu/PeterAde">Peter Ade</a><script data-card-contents-for-user="5463980" type="text/json">{"id":5463980,"first_name":"Peter","last_name":"Ade","domain_name":"independent","page_name":"PeterAde","display_name":"Peter Ade","profile_url":"https://independent.academia.edu/PeterAde?f_ri=15306","photo":"https://0.academia-photos.com/5463980/2398998/2792431/s65_peter.ade.jpg"}</script></span></span></li><li class="js-paper-rank-work_4440853 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="4440853"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 4440853, container: ".js-paper-rank-work_4440853", }); 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$(".js-view-count[data-work-id=4440853]").text(description); $(".js-view-count-work_4440853").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_4440853").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="4440853"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">5</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="1140559" href="https://www.academia.edu/Documents/in/Field_of_View">Field of View</a>, <script data-card-contents-for-ri="1140559" type="text/json">{"id":1140559,"name":"Field of View","url":"https://www.academia.edu/Documents/in/Field_of_View?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="1181678" href="https://www.academia.edu/Documents/in/High_Efficiency">High Efficiency</a>, <script data-card-contents-for-ri="1181678" type="text/json">{"id":1181678,"name":"High Efficiency","url":"https://www.academia.edu/Documents/in/High_Efficiency?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="1358284" href="https://www.academia.edu/Documents/in/Spectral_Resolution">Spectral Resolution</a><script data-card-contents-for-ri="1358284" type="text/json">{"id":1358284,"name":"Spectral Resolution","url":"https://www.academia.edu/Documents/in/Spectral_Resolution?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=4440853]'), work: {"id":4440853,"title":"Herschel-SPIRE: design, performance, and scientific capabilities","created_at":"2013-09-08T23:52:26.608-07:00","url":"https://www.academia.edu/4440853/Herschel_SPIRE_design_performance_and_scientific_capabilities?f_ri=15306","dom_id":"work_4440853","summary":"SPIRE, the Spectral and Photometric Imaging Receiver, is a submillimetre camera and spectrometer for the European Space Agency's Herschel Space Observatory. It comprises a three-band imaging photometer operating at 250, 360 and 520 μm, and an imaging Fourier Transform Spectrometer (FTS) covering 200-670 μm. The detectors are arrays of feedhorn-coupled NTD spider-web bolometers cooled to 0.3 K. The photometer field of view of is 4 x 8 arcmin., observed simultaneously in the three spectral bands. The FTS has an approximately circular field of view with a diameter of 2.6 arcmin., and employs a dual-beam configuration with broad-band intensity beam dividers to provide high efficiency and separated output and input ports. The spectral resolution can be adjusted between 0.04 and 2 cm-1 (resolving power of 20-1000 at 250 μm). The flight instrument is currently undergoing integration and test. The design of SPIRE is described, and the expected scientific performance is summarised, based on modelling and flight instrument test results.","downloadable_attachments":[{"id":49859171,"asset_id":4440853,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":5463980,"first_name":"Peter","last_name":"Ade","domain_name":"independent","page_name":"PeterAde","display_name":"Peter Ade","profile_url":"https://independent.academia.edu/PeterAde?f_ri=15306","photo":"https://0.academia-photos.com/5463980/2398998/2792431/s65_peter.ade.jpg"}],"research_interests":[{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":1140559,"name":"Field of View","url":"https://www.academia.edu/Documents/in/Field_of_View?f_ri=15306","nofollow":false},{"id":1181678,"name":"High Efficiency","url":"https://www.academia.edu/Documents/in/High_Efficiency?f_ri=15306","nofollow":false},{"id":1358284,"name":"Spectral Resolution","url":"https://www.academia.edu/Documents/in/Spectral_Resolution?f_ri=15306","nofollow":false},{"id":1487572,"name":"Space Telescopes","url":"https://www.academia.edu/Documents/in/Space_Telescopes?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_13767041" data-work_id="13767041" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/13767041/Millimetron_a_large_Russian_European_submillimeter_space_observatory">Millimetron—a large Russian-European submillimeter space observatory</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/13767041" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="e8fc30ff1132f933095b2d7593d78382" rel="nofollow" data-download="{"attachment_id":44976257,"asset_id":13767041,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/44976257/download_file?st=MTczMzI2NjQ0MSw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="32879402" href="https://independent.academia.edu/ROrfei">R. 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href="https://www.academia.edu/27484209/GOODS_Herschel_A_population_of_24micron_dropout_sources_at_z_2">GOODS-Herschel A population of 24micron dropout sources at z< 2</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">Abstract: Using extremely deep PACS 100-and 160um Herschel data from the GOODS-Herschel program, we identify 21 infrared bright galaxies previously missed in the deepest 24um surveys performed by MIPS. These MIPS dropouts are... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_27484209" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Abstract: Using extremely deep PACS 100-and 160um Herschel data from the GOODS-Herschel program, we identify 21 infrared bright galaxies previously missed in the deepest 24um surveys performed by MIPS. These MIPS dropouts are predominantly found in two redshift bins, centred at z~ 0.4 and~ 1.3. Their S_100/S_24 flux density ratios are similar to those of local LIRGs and ULIRGs, whose silicate absorption features at 18um (at z~ 0.4) and 9.7 um (at z~ 1.3) are shifted into the 24um MIPS band at these redshifts. 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href="https://www.academia.edu/10510248/A_report_on_the_laboratory_performance_of_the_spectroscopic_detector_arrays_for_SPIRE_HSO">A report on the laboratory performance of the spectroscopic detector arrays for SPIRE/HSO</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">We report the performance of the flight bolometer arrays for the Spectral and Photometric Imaging REceiver (SPIRE) instrument to be on board of the Herschel Space Observatory (HSO). We describe the test setup for the flight Bolometric... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_10510248" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">We report the performance of the flight bolometer arrays for the Spectral and Photometric Imaging REceiver (SPIRE) instrument to be on board of the Herschel Space Observatory (HSO). We describe the test setup for the flight Bolometric Detector Assembly (BDA) that allows the characterization of its performance, both dark and optical, in one instrument's cool down. We summarize the laboratory procedure to measure the basic bolometer parameters, optical response time, optical efficiency of bolometer and feedhorn, dark and optical noise, and the overall thermal conductance of the BDA unit. Finally, we present the test results obtained from the two flight units, Spectroscopic Long Wavelength (SLW) and Spectroscopic Short Wavelength (SSW).</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/10510248" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="60473990a1cab2ba24995e1d5aa06b69" rel="nofollow" data-download="{"attachment_id":47337210,"asset_id":10510248,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/47337210/download_file?st=MTczMzI2NjQ0MSw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="25769947" href="https://independent.academia.edu/VIKTORHRISTOV1">VIKTOR HRISTOV</a><script data-card-contents-for-user="25769947" type="text/json">{"id":25769947,"first_name":"VIKTOR","last_name":"HRISTOV","domain_name":"independent","page_name":"VIKTORHRISTOV1","display_name":"VIKTOR HRISTOV","profile_url":"https://independent.academia.edu/VIKTORHRISTOV1?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_10510248 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="10510248"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 10510248, container: ".js-paper-rank-work_10510248", }); 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Finally, we present the test results obtained from the two flight units, Spectroscopic Long Wavelength (SLW) and Spectroscopic Short Wavelength (SSW).","downloadable_attachments":[{"id":47337210,"asset_id":10510248,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":25769947,"first_name":"VIKTOR","last_name":"HRISTOV","domain_name":"independent","page_name":"VIKTORHRISTOV1","display_name":"VIKTOR HRISTOV","profile_url":"https://independent.academia.edu/VIKTORHRISTOV1?f_ri=15306","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":246758,"name":"Thermal Conductivity","url":"https://www.academia.edu/Documents/in/Thermal_Conductivity?f_ri=15306","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_14287936" data-work_id="14287936" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/14287936/Millimeter_Wave_and_Terahertz_Spectra_of_C_13_Methanol">Millimeter Wave and Terahertz Spectra of C-13 Methanol</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/14287936" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="8713e8a4f12e4ca288d2d50dac305dab" rel="nofollow" data-download="{"attachment_id":44353932,"asset_id":14287936,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/44353932/download_file?st=MTczMzI2NjQ0MSw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="33251296" href="https://newbrunswick.academia.edu/LihongXu">Li-hong Xu</a><script data-card-contents-for-user="33251296" type="text/json">{"id":33251296,"first_name":"Li-hong","last_name":"Xu","domain_name":"newbrunswick","page_name":"LihongXu","display_name":"Li-hong Xu","profile_url":"https://newbrunswick.academia.edu/LihongXu?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_14287936 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="14287936"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 14287936, container: ".js-paper-rank-work_14287936", }); 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THE SMALL MAGELLANIC CLOUD","created_at":"2015-12-07T01:23:24.298-08:00","url":"https://www.academia.edu/19531946/A_SPITZER_SPACE_TELESCOPE_FAR_INFRARED_SPECTRAL_ATLAS_OF_COMPACT_SOURCES_IN_THE_MAGELLANIC_CLOUDS_II_THE_SMALL_MAGELLANIC_CLOUD?f_ri=15306","dom_id":"work_19531946","summary":null,"downloadable_attachments":[{"id":40677316,"asset_id":19531946,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":39843014,"first_name":"Joana","last_name":"Oliveira","domain_name":"independent","page_name":"JoanaOliveira44","display_name":"Joana Oliveira","profile_url":"https://independent.academia.edu/JoanaOliveira44?f_ri=15306","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":321836,"name":"Spectrum","url":"https://www.academia.edu/Documents/in/Spectrum?f_ri=15306","nofollow":false},{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306","nofollow":false},{"id":345043,"name":"Small Magellanic Cloud","url":"https://www.academia.edu/Documents/in/Small_Magellanic_Cloud?f_ri=15306","nofollow":false},{"id":1341823,"name":"Large Magellanic Cloud","url":"https://www.academia.edu/Documents/in/Large_Magellanic_Cloud?f_ri=15306"},{"id":1460347,"name":"Astronomical","url":"https://www.academia.edu/Documents/in/Astronomical?f_ri=15306"},{"id":2217031,"name":"Spectral Energy Distribution","url":"https://www.academia.edu/Documents/in/Spectral_Energy_Distribution?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_19085440 coauthored" data-work_id="19085440" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/19085440/The_Vega_debris_disc_A_view_from_Herschel">The Vega debris disc: A view from Herschel</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/19085440" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="34d066dadf73f4d3e2ce031a58b847d3" rel="nofollow" data-download="{"attachment_id":40422659,"asset_id":19085440,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/40422659/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="39268431" href="https://independent.academia.edu/SRegibo">Sara Regibo</a><script data-card-contents-for-user="39268431" type="text/json">{"id":39268431,"first_name":"Sara","last_name":"Regibo","domain_name":"independent","page_name":"SRegibo","display_name":"Sara Regibo","profile_url":"https://independent.academia.edu/SRegibo?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span><span class="u-displayInlineBlock InlineList-item-text"> and <span class="u-textDecorationUnderline u-clickable InlineList-item-text js-work-more-authors-19085440">+1</span><div class="hidden js-additional-users-19085440"><div><span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a href="https://independent.academia.edu/WMeester">Wim De Meester</a></span></div></div></span><script>(function(){ var popoverSettings = { el: $('.js-work-more-authors-19085440'), placement: 'bottom', hide_delay: 200, html: true, content: function(){ return $('.js-additional-users-19085440').html(); 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We also make... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_38740040" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Using deep 100-160 micron observations in GOODS-S from the GOODS-H survey, combined with HST/WFC3 NIR imaging from CANDELS, we present the first morphological analysis of a complete, FIR selected sample of 52 ULIRGs at z~2. We also make use of a comparison sample of galaxies without Herschel detections but with the same z and magnitude distribution. Our visual classifications of</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/38740040" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="8ca24ccd902b6fae31bba2529ac3f94c" rel="nofollow" data-download="{"attachment_id":58827317,"asset_id":38740040,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/58827317/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="107908210" href="https://independent.academia.edu/RayLucas5">Ray Lucas</a><script data-card-contents-for-user="107908210" type="text/json">{"id":107908210,"first_name":"Ray","last_name":"Lucas","domain_name":"independent","page_name":"RayLucas5","display_name":"Ray Lucas","profile_url":"https://independent.academia.edu/RayLucas5?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_38740040 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="38740040"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 38740040, container: ".js-paper-rank-work_38740040", }); 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$(".js-view-count[data-work-id=38740040]").text(description); $(".js-view-count-work_38740040").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_38740040").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="38740040"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">5</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="11050" href="https://www.academia.edu/Documents/in/Galaxy_Formation_and_Evolution">Galaxy Formation and Evolution</a>, <script data-card-contents-for-ri="11050" type="text/json">{"id":11050,"name":"Galaxy Formation and Evolution","url":"https://www.academia.edu/Documents/in/Galaxy_Formation_and_Evolution?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="149520" href="https://www.academia.edu/Documents/in/Morphological_Analysis">Morphological Analysis</a>, <script data-card-contents-for-ri="149520" type="text/json">{"id":149520,"name":"Morphological Analysis","url":"https://www.academia.edu/Documents/in/Morphological_Analysis?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="335361" href="https://www.academia.edu/Documents/in/Infrared">Infrared</a><script data-card-contents-for-ri="335361" type="text/json">{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=38740040]'), work: {"id":38740040,"title":"GOODS-Herschel \u0026 CANDELS: The Morphologies of Ultraluminous Infrared Galaxies at z~2","created_at":"2019-04-08T04:30:38.310-07:00","url":"https://www.academia.edu/38740040/GOODS_Herschel_and_CANDELS_The_Morphologies_of_Ultraluminous_Infrared_Galaxies_at_z_2?f_ri=15306","dom_id":"work_38740040","summary":"Using deep 100-160 micron observations in GOODS-S from the GOODS-H survey, combined with HST/WFC3 NIR imaging from CANDELS, we present the first morphological analysis of a complete, FIR selected sample of 52 ULIRGs at z~2. We also make use of a comparison sample of galaxies without Herschel detections but with the same z and magnitude distribution. Our visual classifications of","downloadable_attachments":[{"id":58827317,"asset_id":38740040,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":107908210,"first_name":"Ray","last_name":"Lucas","domain_name":"independent","page_name":"RayLucas5","display_name":"Ray Lucas","profile_url":"https://independent.academia.edu/RayLucas5?f_ri=15306","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":11050,"name":"Galaxy Formation and Evolution","url":"https://www.academia.edu/Documents/in/Galaxy_Formation_and_Evolution?f_ri=15306","nofollow":false},{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":149520,"name":"Morphological Analysis","url":"https://www.academia.edu/Documents/in/Morphological_Analysis?f_ri=15306","nofollow":false},{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306","nofollow":false},{"id":2741909,"name":"Selective Sampling","url":"https://www.academia.edu/Documents/in/Selective_Sampling?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_35609636 coauthored" data-work_id="35609636" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/35609636/Inventing_a_Space_Mission_The_Story_of_the_Herschel_Space_Observatory">Inventing a Space Mission: The Story of the Herschel Space Observatory</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">This book describes prominent technological achievements within a very successful space science mission: the Herschel space observatory. Focusing on the various processes of innovation it offers an analysis and discussion of the social,... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_35609636" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">This book describes prominent technological achievements within a very successful space science mission: the Herschel space observatory. Focusing on the various processes of innovation it offers an analysis and discussion of the social, technological and scientific context of the mission that paved the way to its development. It addresses the key question raised by these processes in our modern society, i.e.: how knowledge management of innovation set the conditions for inventing the future? In that respect the book is based on a transdisciplinary analysis of the programmatic complexity of Herschel, with inputs from space scientists, managers, philosophers, and engineers.<br /><br />This book is addressed to decision makers, not only in space science, but also in other industries and sciences using or building large machines. It is also addressed to space engineers and scientists as well as students in science and management.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/35609636" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="8faec85872f4e081b2604e4caecab01a" rel="nofollow" data-download="{"attachment_id":55477372,"asset_id":35609636,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/55477372/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="8362053" href="https://cea.academia.edu/VincentBontems">Vincent Bontems</a><script data-card-contents-for-user="8362053" type="text/json">{"id":8362053,"first_name":"Vincent","last_name":"Bontems","domain_name":"cea","page_name":"VincentBontems","display_name":"Vincent Bontems","profile_url":"https://cea.academia.edu/VincentBontems?f_ri=15306","photo":"https://0.academia-photos.com/8362053/2852605/79628320/s65_vincent.bontems.jpeg"}</script></span></span><span class="u-displayInlineBlock InlineList-item-text"> and <span class="u-textDecorationUnderline u-clickable InlineList-item-text js-work-more-authors-35609636">+1</span><div class="hidden js-additional-users-35609636"><div><span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a href="https://independent.academia.edu/G%C3%B6ranPilbratt">Göran Pilbratt</a></span></div></div></span><script>(function(){ var popoverSettings = { el: $('.js-work-more-authors-35609636'), placement: 'bottom', hide_delay: 200, html: true, content: function(){ return $('.js-additional-users-35609636').html(); 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Focusing on the various processes of innovation it offers an analysis and discussion of the social, technological and scientific context of the mission that paved the way to its development. It addresses the key question raised by these processes in our modern society, i.e.: how knowledge management of innovation set the conditions for inventing the future? In that respect the book is based on a transdisciplinary analysis of the programmatic complexity of Herschel, with inputs from space scientists, managers, philosophers, and engineers.\n\nThis book is addressed to decision makers, not only in space science, but also in other industries and sciences using or building large machines. It is also addressed to space engineers and scientists as well as students in science and management.","downloadable_attachments":[{"id":55477372,"asset_id":35609636,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":8362053,"first_name":"Vincent","last_name":"Bontems","domain_name":"cea","page_name":"VincentBontems","display_name":"Vincent Bontems","profile_url":"https://cea.academia.edu/VincentBontems?f_ri=15306","photo":"https://0.academia-photos.com/8362053/2852605/79628320/s65_vincent.bontems.jpeg"},{"id":74538279,"first_name":"Göran","last_name":"Pilbratt","domain_name":"independent","page_name":"GöranPilbratt","display_name":"Göran Pilbratt","profile_url":"https://independent.academia.edu/G%C3%B6ranPilbratt?f_ri=15306","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":1404,"name":"Creativity--Knowledge Invention \u0026 Discovery","url":"https://www.academia.edu/Documents/in/Creativity--Knowledge_Invention_and_Discovery?f_ri=15306","nofollow":false},{"id":7831,"name":"Management of Innovation","url":"https://www.academia.edu/Documents/in/Management_of_Innovation?f_ri=15306","nofollow":false},{"id":8298,"name":"Gilbert Simondon","url":"https://www.academia.edu/Documents/in/Gilbert_Simondon?f_ri=15306","nofollow":false},{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":16091,"name":"Sociology of Science","url":"https://www.academia.edu/Documents/in/Sociology_of_Science?f_ri=15306"},{"id":23179,"name":"Astrophysics","url":"https://www.academia.edu/Documents/in/Astrophysics?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_27502400" data-work_id="27502400" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/27502400/The_Herschel_and_Planck_Space_Telescopes">The Herschel and Planck Space Telescopes</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/27502400" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="2634226d2690573d331363e244255f3f" rel="nofollow" data-download="{"attachment_id":47758715,"asset_id":27502400,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/47758715/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="51656425" href="https://independent.academia.edu/TauberJ">J. 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href="https://www.academia.edu/10005331/The_Herschel_Heterodyne_Instrument_for_the_Far_Infrared_HIFI_instrument_and_pre_launch_testing">The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI): instrument and pre-launch testing</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/10005331" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="b5a6d7b37f7e713d33b6c85995c3bc9f" rel="nofollow" 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(Astronomy \u0026 Astrophysics)","url":"https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="47599" href="https://www.academia.edu/Documents/in/Astronomy">Astronomy</a><script data-card-contents-for-ri="47599" type="text/json">{"id":47599,"name":"Astronomy","url":"https://www.academia.edu/Documents/in/Astronomy?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=10005331]'), work: 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href="https://www.academia.edu/14538043/HERSCHEL_OBSERVATIONS_OF_EXTRAORDINARY_SOURCES_ANALYSIS_OF_THE_HIFI_1_2_THz_WIDE_SPECTRAL_SURVEY_TOWARD_ORION_KL_I_METHODS">HERSCHEL OBSERVATIONS OF EXTRAORDINARY SOURCES: ANALYSIS OF THE HIFI 1.2 THz WIDE SPECTRAL SURVEY TOWARD ORION KL. I. METHODS</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/14538043" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="8d8d3fcfe434759969f16d2f1b6a6b31" rel="nofollow" data-download="{"attachment_id":44084415,"asset_id":14538043,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/44084415/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="33496985" href="https://independent.academia.edu/McGuireBrett">Brett McGuire</a><script data-card-contents-for-user="33496985" type="text/json">{"id":33496985,"first_name":"Brett","last_name":"McGuire","domain_name":"independent","page_name":"McGuireBrett","display_name":"Brett McGuire","profile_url":"https://independent.academia.edu/McGuireBrett?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_14538043 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="14538043"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 14538043, container: ".js-paper-rank-work_14538043", }); 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js-work-card work_15001958 coauthored" data-work_id="15001958" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/15001958/The_Herschel_SPIRE_instrument_and_its_in_flight_performance">The Herschel -SPIRE instrument and its in-flight performance</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/15001958" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="123d13ddf03415db872061952b797562" rel="nofollow" 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href="https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_">Dust (Astronomy & Astrophysics)</a>, <script data-card-contents-for-ri="11125" type="text/json">{"id":11125,"name":"Dust (Astronomy \u0026 Astrophysics)","url":"https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a><script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=15001958]'), work: {"id":15001958,"title":"The Herschel -SPIRE instrument and its in-flight 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u-pv7x u-mb0x js-work-card work_15093008 coauthored" data-work_id="15093008" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/15093008/Preparation_for_the_solar_system_observations_with_Herschel_Simulation_of_Jupiter_observations_with_PACS">Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/15093008" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" 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Here we examine whether the... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_76140766" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the spectral energy distribution (SED) and dust temperature of galaxies have strongly evolved since z~2.5. We use Herschel deep extragalactic surveys from 100 to 500um to compute total IR luminosities in galaxies down to the faintest levels, using PACS and SPIRE in the GOODS-North field (PEP and HerMES key programs). We show that measurements in the SPIRE bands can be used below the statistical confusion limit if information at higher spatial resolution is used to identify isolated galaxies whose flux is not boosted by bright neighbors. Below z~1.5, mid-IR extrapolations are correct for star-forming galaxies with a dispersion of only 40% (0.15dex), therefore similar to z~0 galaxies. This narrow distribution is puzzling when considering the range of physic...</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/76140766" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="fcb91b2362f13f538efdce04d1ffc169" rel="nofollow" data-download="{"attachment_id":83807503,"asset_id":76140766,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/83807503/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="7771599" href="https://independent.academia.edu/Zacar%C3%ADasIsmaelP%C3%A9rezCalderon">Zacarías Ismael Pérez Calderon</a><script data-card-contents-for-user="7771599" type="text/json">{"id":7771599,"first_name":"Zacarías Ismael","last_name":"Pérez Calderon","domain_name":"independent","page_name":"ZacaríasIsmaelPérezCalderon","display_name":"Zacarías Ismael Pérez Calderon","profile_url":"https://independent.academia.edu/Zacar%C3%ADasIsmaelP%C3%A9rezCalderon?f_ri=15306","photo":"https://0.academia-photos.com/7771599/6169131/6991356/s65_zacar_as_ismael.p_rez_calderon.jpg_oh_868034dd42161db618e19422d23e818e_oe_55160f1b___gda___1428158447_4511a3d30048ab85c1caa12bc1e7b0c4"}</script></span></span></li><li class="js-paper-rank-work_76140766 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="76140766"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 76140766, container: ".js-paper-rank-work_76140766", }); 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This narrow distribution is puzzling when considering the range of physic...","downloadable_attachments":[{"id":83807503,"asset_id":76140766,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":7771599,"first_name":"Zacarías Ismael","last_name":"Pérez Calderon","domain_name":"independent","page_name":"ZacaríasIsmaelPérezCalderon","display_name":"Zacarías Ismael Pérez Calderon","profile_url":"https://independent.academia.edu/Zacar%C3%ADasIsmaelP%C3%A9rezCalderon?f_ri=15306","photo":"https://0.academia-photos.com/7771599/6169131/6991356/s65_zacar_as_ismael.p_rez_calderon.jpg_oh_868034dd42161db618e19422d23e818e_oe_55160f1b___gda___1428158447_4511a3d30048ab85c1caa12bc1e7b0c4"}],"research_interests":[{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=15306","nofollow":false},{"id":4363,"name":"Star Formation","url":"https://www.academia.edu/Documents/in/Star_Formation?f_ri=15306","nofollow":false},{"id":4742,"name":"Active Galactic Nuclei","url":"https://www.academia.edu/Documents/in/Active_Galactic_Nuclei?f_ri=15306","nofollow":false},{"id":11125,"name":"Dust (Astronomy \u0026 Astrophysics)","url":"https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_?f_ri=15306","nofollow":false},{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306"},{"id":97563,"name":"Galaxy evolution","url":"https://www.academia.edu/Documents/in/Galaxy_evolution?f_ri=15306"},{"id":335363,"name":"Far Infrared","url":"https://www.academia.edu/Documents/in/Far_Infrared?f_ri=15306"},{"id":423611,"name":"Active Galaxies","url":"https://www.academia.edu/Documents/in/Active_Galaxies?f_ri=15306"},{"id":482037,"name":"Partituras E Músicas","url":"https://www.academia.edu/Documents/in/Partituras_E_Musicas?f_ri=15306"},{"id":604200,"name":"Spatial resolution","url":"https://www.academia.edu/Documents/in/Spatial_resolution?f_ri=15306"},{"id":977447,"name":"Starburst Galaxies","url":"https://www.academia.edu/Documents/in/Starburst_Galaxies?f_ri=15306"},{"id":2217031,"name":"Spectral Energy Distribution","url":"https://www.academia.edu/Documents/in/Spectral_Energy_Distribution?f_ri=15306"},{"id":3243321,"name":"Principal Investigator","url":"https://www.academia.edu/Documents/in/Principal_Investigator?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_74723302" data-work_id="74723302" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/74723302/Laboratory_Spectrum_of_the_111_202Rotational_Transition_of_CH2">Laboratory Spectrum of the 111–202Rotational Transition of CH2</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/74723302" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="137575209" href="https://uchile.academia.edu/Michael">Ernest Michael</a><script data-card-contents-for-user="137575209" type="text/json">{"id":137575209,"first_name":"Ernest","last_name":"Michael","domain_name":"uchile","page_name":"Michael","display_name":"Ernest Michael","profile_url":"https://uchile.academia.edu/Michael?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_74723302 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="74723302"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 74723302, container: ".js-paper-rank-work_74723302", }); 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ALMA... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_70047950" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">In the far-infrared (FIR) / THz regime the angular (and often spectral) resolution of observing facilities is still very restricted despite the fact that this frequency range has become of prime importance for modern astrophysics. ALMA (Atacama Large Millimeter Array) with its superb sensitivity and angular resolution will only cover frequencies up to about 1 THz, while the HIFI instrument for ESA&#x27;s Herschel Space Observatory will provide limited angular resolution (10 to 30 arcsec) up to 2 THz. Observations of regions with star and planet formation require extremely high angular resolution as well as frequency resolution in the full THz regime. In order to open these regions for high-resolution astrophysics we propose a heterodyne space interferometer mission, ESPRIT (Exploratory Submm Space Radio-Interferometric Telescope), for the Terahertz regime inaccessible from ground and outside the operating range of the James Webb Space Telescope (JWST). This interferometer will use c...</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/70047950" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="bfda7f44b6654b40724f0858bf523164" rel="nofollow" data-download="{"attachment_id":79926703,"asset_id":70047950,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/79926703/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="59186376" href="https://utwente.academia.edu/AGunst">A. 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HIFI spectroscopy of NGC 1333</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">'Water In Star-forming regions with Herschel' (WISH) is a key programme dedicated to studying the role of water and related species during the star-formation process and constraining the physical and chemical properties of young stellar... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_7336595" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">'Water In Star-forming regions with Herschel' (WISH) is a key programme dedicated to studying the role of water and related species during the star-formation process and constraining the physical and chemical properties of young stellar objects. The Heterodyne Instrument for the Far-Infrared (HIFI) on the Herschel Space Observatory observed three deeply embedded protostars in the low-mass star-forming region NGC1333 in several H2-16O, H2-18O, and CO transitions. Line profiles are resolved for five H16O transitions in each source, revealing them to be surprisingly complex. The line profiles are decomposed into broad (>20 km/s), medium-broad (~5-10 km/s), and narrow (<5 km/s) components. The H2-18O emission is only detected in broad 1_10-1_01 lines (>20 km/s), indicating that its physical origin is the same as for the broad H2-16O component. In one of the sources, IRAS4A, an inverse P Cygni profile is observed, a clear sign of infall in the envelope. From the line profiles alone, it is clear that the bulk of emission arises from shocks, both on small (<1000 AU) and large scales along the outflow cavity walls (~10 000 AU). The H2O line profiles are compared to CO line profiles to constrain the H2O abundance as a function of velocity within these shocked regions. The H2O/CO abundance ratios are measured to be in the range of ~0.1-1, corresponding to H2O abundances of ~10-5-10-4 with respect to H2. Approximately 5-10% of the gas is hot enough for all oxygen to be driven into water in warm post-shock gas, mostly at high velocities.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/7336595" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="1b2348b62360f9b92691b43357cdf489" rel="nofollow" data-download="{"attachment_id":33939683,"asset_id":7336595,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/33939683/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="9126" href="https://ku-dk.academia.edu/LarsKristensen">Lars Kristensen</a><script data-card-contents-for-user="9126" type="text/json">{"id":9126,"first_name":"Lars","last_name":"Kristensen","domain_name":"ku-dk","page_name":"LarsKristensen","display_name":"Lars Kristensen","profile_url":"https://ku-dk.academia.edu/LarsKristensen?f_ri=15306","photo":"https://0.academia-photos.com/9126/9618811/10714185/s65_lars.kristensen.png"}</script></span></span></li><li class="js-paper-rank-work_7336595 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="7336595"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 7336595, container: ".js-paper-rank-work_7336595", }); 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$(".js-view-count[data-work-id=7336595]").text(description); $(".js-view-count-work_7336595").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_7336595").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="7336595"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">8</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="4363" href="https://www.academia.edu/Documents/in/Star_Formation">Star Formation</a>, <script data-card-contents-for-ri="4363" type="text/json">{"id":4363,"name":"Star Formation","url":"https://www.academia.edu/Documents/in/Star_Formation?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="11125" href="https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_">Dust (Astronomy & Astrophysics)</a>, <script data-card-contents-for-ri="11125" type="text/json">{"id":11125,"name":"Dust (Astronomy \u0026 Astrophysics)","url":"https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="47599" href="https://www.academia.edu/Documents/in/Astronomy">Astronomy</a><script data-card-contents-for-ri="47599" type="text/json">{"id":47599,"name":"Astronomy","url":"https://www.academia.edu/Documents/in/Astronomy?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=7336595]'), work: {"id":7336595,"title":"Water in low-mass star-forming regions with Herschel . HIFI spectroscopy of NGC 1333","created_at":"2014-06-13T03:28:18.264-07:00","url":"https://www.academia.edu/7336595/Water_in_low_mass_star_forming_regions_with_Herschel_HIFI_spectroscopy_of_NGC_1333?f_ri=15306","dom_id":"work_7336595","summary":"'Water In Star-forming regions with Herschel' (WISH) is a key programme dedicated to studying the role of water and related species during the star-formation process and constraining the physical and chemical properties of young stellar objects. The Heterodyne Instrument for the Far-Infrared (HIFI) on the Herschel Space Observatory observed three deeply embedded protostars in the low-mass star-forming region NGC1333 in several H2-16O, H2-18O, and CO transitions. Line profiles are resolved for five H16O transitions in each source, revealing them to be surprisingly complex. The line profiles are decomposed into broad (\u003e20 km/s), medium-broad (~5-10 km/s), and narrow (\u003c5 km/s) components. The H2-18O emission is only detected in broad 1_10-1_01 lines (\u003e20 km/s), indicating that its physical origin is the same as for the broad H2-16O component. In one of the sources, IRAS4A, an inverse P Cygni profile is observed, a clear sign of infall in the envelope. From the line profiles alone, it is clear that the bulk of emission arises from shocks, both on small (\u003c1000 AU) and large scales along the outflow cavity walls (~10 000 AU). The H2O line profiles are compared to CO line profiles to constrain the H2O abundance as a function of velocity within these shocked regions. The H2O/CO abundance ratios are measured to be in the range of ~0.1-1, corresponding to H2O abundances of ~10-5-10-4 with respect to H2. Approximately 5-10% of the gas is hot enough for all oxygen to be driven into water in warm post-shock gas, mostly at high velocities.","downloadable_attachments":[{"id":33939683,"asset_id":7336595,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":9126,"first_name":"Lars","last_name":"Kristensen","domain_name":"ku-dk","page_name":"LarsKristensen","display_name":"Lars Kristensen","profile_url":"https://ku-dk.academia.edu/LarsKristensen?f_ri=15306","photo":"https://0.academia-photos.com/9126/9618811/10714185/s65_lars.kristensen.png"}],"research_interests":[{"id":4363,"name":"Star Formation","url":"https://www.academia.edu/Documents/in/Star_Formation?f_ri=15306","nofollow":false},{"id":11125,"name":"Dust (Astronomy \u0026 Astrophysics)","url":"https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_?f_ri=15306","nofollow":false},{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":47599,"name":"Astronomy","url":"https://www.academia.edu/Documents/in/Astronomy?f_ri=15306","nofollow":false},{"id":335363,"name":"Far Infrared","url":"https://www.academia.edu/Documents/in/Far_Infrared?f_ri=15306"},{"id":535357,"name":"Low Mass Stars","url":"https://www.academia.edu/Documents/in/Low_Mass_Stars?f_ri=15306"},{"id":704293,"name":"Chemical Properties","url":"https://www.academia.edu/Documents/in/Chemical_Properties?f_ri=15306"},{"id":758278,"name":"Large Scale","url":"https://www.academia.edu/Documents/in/Large_Scale?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_7921981" data-work_id="7921981" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/7921981/Gas_in_Protoplanetary_Discs_GASPS_1_First_results">Gas in Protoplanetary Discs (GASPS) 1. First results</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the study of the warm disc atmosphere, using far-infrared... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_7921981" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the study of the warm disc atmosphere, using far-infrared spectroscopy to measure gas content and excitation conditions, and far-IR photometry to constrain the dust distribution. Aims - We aim to detect and characterize the gas content of circumstellar discs in four targets as part of the Herschel science demonstration phase. Methods - We carried out sensitive medium resolution spectroscopy and high sensitivity photometry at lambda ~60-190 micron using the Photodetector Array Camera and Spectrometer instrument on the Herschel space observatory. Results - We detect [OI] 63 micron emission from the young stars HD 169142, TW Hydrae, and RECX 15, but not HD 181327. No other lines, including [CII] 158 and [OI] 145, are significantly detected. All four stars are detected in photometry at 70 and 160 micron. Extensive models are presented in associated papers.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/7921981" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="c989f0c6d72ff35662bd2562aec082be" rel="nofollow" data-download="{"attachment_id":34400678,"asset_id":7921981,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/34400678/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="14870042" href="https://goldsmiths.academia.edu/NicolaBrittain">Nicola Brittain</a><script data-card-contents-for-user="14870042" type="text/json">{"id":14870042,"first_name":"Nicola","last_name":"Brittain","domain_name":"goldsmiths","page_name":"NicolaBrittain","display_name":"Nicola Brittain","profile_url":"https://goldsmiths.academia.edu/NicolaBrittain?f_ri=15306","photo":"https://0.academia-photos.com/14870042/4053761/4729345/s65_nicola.brittain.jpg"}</script></span></span></li><li class="js-paper-rank-work_7921981 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="7921981"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 7921981, container: ".js-paper-rank-work_7921981", }); });</script></li><li class="js-percentile-work_7921981 InlineList-item InlineList-item--bordered hidden u-tcGrayDark"><span class="percentile-widget hidden"><span class="u-mr2x percentile-widget" style="display: none">•</span><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 7921981; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-percentile-work_7921981"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></li><li class="js-view-count-work_7921981 InlineList-item InlineList-item--bordered hidden"><div><span><span class="js-view-count view-count u-mr2x" data-work-id="7921981"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 7921981; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=7921981]").text(description); $(".js-view-count-work_7921981").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_7921981").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="7921981"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">6</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="195544" href="https://www.academia.edu/Documents/in/Planetary_Systems">Planetary Systems</a>, <script data-card-contents-for-ri="195544" type="text/json">{"id":195544,"name":"Planetary Systems","url":"https://www.academia.edu/Documents/in/Planetary_Systems?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="335361" href="https://www.academia.edu/Documents/in/Infrared">Infrared</a>, <script data-card-contents-for-ri="335361" type="text/json">{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="335363" href="https://www.academia.edu/Documents/in/Far_Infrared">Far Infrared</a><script data-card-contents-for-ri="335363" type="text/json">{"id":335363,"name":"Far Infrared","url":"https://www.academia.edu/Documents/in/Far_Infrared?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=7921981]'), work: {"id":7921981,"title":"Gas in Protoplanetary Discs (GASPS) 1. First results","created_at":"2014-08-08T16:29:48.299-07:00","url":"https://www.academia.edu/7921981/Gas_in_Protoplanetary_Discs_GASPS_1_First_results?f_ri=15306","dom_id":"work_7921981","summary":"Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the study of the warm disc atmosphere, using far-infrared spectroscopy to measure gas content and excitation conditions, and far-IR photometry to constrain the dust distribution. Aims - We aim to detect and characterize the gas content of circumstellar discs in four targets as part of the Herschel science demonstration phase. Methods - We carried out sensitive medium resolution spectroscopy and high sensitivity photometry at lambda ~60-190 micron using the Photodetector Array Camera and Spectrometer instrument on the Herschel space observatory. Results - We detect [OI] 63 micron emission from the young stars HD 169142, TW Hydrae, and RECX 15, but not HD 181327. No other lines, including [CII] 158 and [OI] 145, are significantly detected. All four stars are detected in photometry at 70 and 160 micron. Extensive models are presented in associated papers.","downloadable_attachments":[{"id":34400678,"asset_id":7921981,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":14870042,"first_name":"Nicola","last_name":"Brittain","domain_name":"goldsmiths","page_name":"NicolaBrittain","display_name":"Nicola Brittain","profile_url":"https://goldsmiths.academia.edu/NicolaBrittain?f_ri=15306","photo":"https://0.academia-photos.com/14870042/4053761/4729345/s65_nicola.brittain.jpg"}],"research_interests":[{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":195544,"name":"Planetary Systems","url":"https://www.academia.edu/Documents/in/Planetary_Systems?f_ri=15306","nofollow":false},{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306","nofollow":false},{"id":335363,"name":"Far Infrared","url":"https://www.academia.edu/Documents/in/Far_Infrared?f_ri=15306","nofollow":false},{"id":951921,"name":"Pre main Sequence Stars","url":"https://www.academia.edu/Documents/in/Pre_main_Sequence_Stars?f_ri=15306"},{"id":962638,"name":"High Sensitivity","url":"https://www.academia.edu/Documents/in/High_Sensitivity?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_9299021" data-work_id="9299021" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/9299021/The_data_processing_pipelines_for_the_Herschel_SPIRE_imaging_Fourier_transform_spectrometer">The data processing pipelines for the Herschel/SPIRE imaging Fourier transform spectrometer</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">We present an update to the data processing pipelines that generate calibrated spectral data products from the Spectral and Photometric Imaging Receiver (SPIRE), one of three scientific instruments onboard the European Space Agency's... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_9299021" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">We present an update to the data processing pipelines that generate calibrated spectral data products from the Spectral and Photometric Imaging Receiver (SPIRE), one of three scientific instruments onboard the European Space Agency's Herschel Space Observatory launched on 14 May 2009. The pipelines process telemetry from SPIRE's imaging Fourier Transform Spectrometer (FTS) taken in point source, jiggle- and raster-map observing modes, producing calibrated spectra in low-, medium-, high-, and mixed low- and high-spectral resolution. While the order and algorithms of the data processing modules in the spectrometer pipelines remain for the most part unchanged compared to their pre-launch status, some improvements and optimizations have been realized through the analysis of data from the performance verification and science demonstration phases of the mission. The data processing pipelines for the SPIRE FTS as of the beginning of the routine phase of the Herschel mission are presented in their entirety, with more detailed descriptions reserved for those elements that have changed since launch, in particular the first- and second-level correction steps for glitches, the step that corrects for clipped samples, and the process by which Level-1 spectral data are converted to Level-2 products. In addition, we discuss some of the challenging aspects still faced by the automated processing pipelines, such as the removal of the contributions from the Herschel telescope and SPIRE instrument, and the relative spectral response correction and flux conversion steps.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/9299021" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="cb87e70d6a7d849362c8e6fbf068c7a0" rel="nofollow" data-download="{"attachment_id":47828557,"asset_id":9299021,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/47828557/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="21431453" href="https://lam.academia.edu/ChristianSurace">Christian Surace</a><script data-card-contents-for-user="21431453" type="text/json">{"id":21431453,"first_name":"Christian","last_name":"Surace","domain_name":"lam","page_name":"ChristianSurace","display_name":"Christian Surace","profile_url":"https://lam.academia.edu/ChristianSurace?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_9299021 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="9299021"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 9299021, container: ".js-paper-rank-work_9299021", }); 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The pipelines process telemetry from SPIRE's imaging Fourier Transform Spectrometer (FTS) taken in point source, jiggle- and raster-map observing modes, producing calibrated spectra in low-, medium-, high-, and mixed low- and high-spectral resolution. While the order and algorithms of the data processing modules in the spectrometer pipelines remain for the most part unchanged compared to their pre-launch status, some improvements and optimizations have been realized through the analysis of data from the performance verification and science demonstration phases of the mission. The data processing pipelines for the SPIRE FTS as of the beginning of the routine phase of the Herschel mission are presented in their entirety, with more detailed descriptions reserved for those elements that have changed since launch, in particular the first- and second-level correction steps for glitches, the step that corrects for clipped samples, and the process by which Level-1 spectral data are converted to Level-2 products. In addition, we discuss some of the challenging aspects still faced by the automated processing pipelines, such as the removal of the contributions from the Herschel telescope and SPIRE instrument, and the relative spectral response correction and flux conversion steps.","downloadable_attachments":[{"id":47828557,"asset_id":9299021,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":21431453,"first_name":"Christian","last_name":"Surace","domain_name":"lam","page_name":"ChristianSurace","display_name":"Christian Surace","profile_url":"https://lam.academia.edu/ChristianSurace?f_ri=15306","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":40276,"name":"Proceedings","url":"https://www.academia.edu/Documents/in/Proceedings?f_ri=15306","nofollow":false},{"id":581652,"name":"Data Processing","url":"https://www.academia.edu/Documents/in/Data_Processing?f_ri=15306","nofollow":false},{"id":1114258,"name":"Level","url":"https://www.academia.edu/Documents/in/Level?f_ri=15306","nofollow":false},{"id":1358284,"name":"Spectral Resolution","url":"https://www.academia.edu/Documents/in/Spectral_Resolution?f_ri=15306"},{"id":2506762,"name":"Spectral Response","url":"https://www.academia.edu/Documents/in/Spectral_Response?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_27022452" data-work_id="27022452" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/27022452/GOODS_Herschel_and_CANDELS_The_Morphologies_of_Ultraluminous_Infrared_Galaxies_at_z_2">GOODS-Herschel & CANDELS: The Morphologies of Ultraluminous Infrared Galaxies at z~2</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">Using deep 100-160 micron observations in GOODS-S from the GOODS-H survey, combined with HST/WFC3 NIR imaging from CANDELS, we present the first morphological analysis of a complete, FIR selected sample of 52 ULIRGs at z~2. We also make... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_27022452" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Using deep 100-160 micron observations in GOODS-S from the GOODS-H survey, combined with HST/WFC3 NIR imaging from CANDELS, we present the first morphological analysis of a complete, FIR selected sample of 52 ULIRGs at z~2. We also make use of a comparison sample of galaxies without Herschel detections but with the same z and magnitude distribution. Our visual classifications of</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/27022452" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="604bf1db5739b7805d247352ec713533" rel="nofollow" data-download="{"attachment_id":47286074,"asset_id":27022452,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/47286074/download_file?st=MTczMzI2NjQ0Miw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="51053086" href="https://independent.academia.edu/JamesDunlop2">James Dunlop</a><script data-card-contents-for-user="51053086" type="text/json">{"id":51053086,"first_name":"James","last_name":"Dunlop","domain_name":"independent","page_name":"JamesDunlop2","display_name":"James Dunlop","profile_url":"https://independent.academia.edu/JamesDunlop2?f_ri=15306","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_27022452 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="27022452"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 27022452, container: ".js-paper-rank-work_27022452", }); 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$(".js-view-count[data-work-id=27022452]").text(description); $(".js-view-count-work_27022452").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_27022452").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="27022452"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">4</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="11050" href="https://www.academia.edu/Documents/in/Galaxy_Formation_and_Evolution">Galaxy Formation and Evolution</a>, <script data-card-contents-for-ri="11050" type="text/json">{"id":11050,"name":"Galaxy Formation and Evolution","url":"https://www.academia.edu/Documents/in/Galaxy_Formation_and_Evolution?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="149520" href="https://www.academia.edu/Documents/in/Morphological_Analysis">Morphological Analysis</a>, <script data-card-contents-for-ri="149520" type="text/json">{"id":149520,"name":"Morphological Analysis","url":"https://www.academia.edu/Documents/in/Morphological_Analysis?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="335361" href="https://www.academia.edu/Documents/in/Infrared">Infrared</a><script data-card-contents-for-ri="335361" type="text/json">{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=27022452]'), work: {"id":27022452,"title":"GOODS-Herschel \u0026 CANDELS: The Morphologies of Ultraluminous Infrared Galaxies at z~2","created_at":"2016-07-15T23:07:23.142-07:00","url":"https://www.academia.edu/27022452/GOODS_Herschel_and_CANDELS_The_Morphologies_of_Ultraluminous_Infrared_Galaxies_at_z_2?f_ri=15306","dom_id":"work_27022452","summary":"Using deep 100-160 micron observations in GOODS-S from the GOODS-H survey, combined with HST/WFC3 NIR imaging from CANDELS, we present the first morphological analysis of a complete, FIR selected sample of 52 ULIRGs at z~2. We also make use of a comparison sample of galaxies without Herschel detections but with the same z and magnitude distribution. Our visual classifications of","downloadable_attachments":[{"id":47286074,"asset_id":27022452,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":51053086,"first_name":"James","last_name":"Dunlop","domain_name":"independent","page_name":"JamesDunlop2","display_name":"James Dunlop","profile_url":"https://independent.academia.edu/JamesDunlop2?f_ri=15306","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":11050,"name":"Galaxy Formation and Evolution","url":"https://www.academia.edu/Documents/in/Galaxy_Formation_and_Evolution?f_ri=15306","nofollow":false},{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":149520,"name":"Morphological 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Analysis","url":"https://www.academia.edu/Documents/in/Global_Analysis?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="41120" href="https://www.academia.edu/Documents/in/Millimeter_Wave_Antennas">Millimeter Wave Antennas</a><script data-card-contents-for-ri="41120" type="text/json">{"id":41120,"name":"Millimeter Wave Antennas","url":"https://www.academia.edu/Documents/in/Millimeter_Wave_Antennas?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=14287875]'), work: {"id":14287875,"title":"Torsion–rotation global analysis of the first three torsional states (νt=0, 1, 2) and terahertz database for 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Analysis","url":"https://www.academia.edu/Documents/in/Global_Analysis?f_ri=15306","nofollow":false},{"id":41120,"name":"Millimeter Wave Antennas","url":"https://www.academia.edu/Documents/in/Millimeter_Wave_Antennas?f_ri=15306","nofollow":false},{"id":50157,"name":"Molecular","url":"https://www.academia.edu/Documents/in/Molecular?f_ri=15306"},{"id":127997,"name":"Terahertz","url":"https://www.academia.edu/Documents/in/Terahertz?f_ri=15306"},{"id":258979,"name":"Computer Program","url":"https://www.academia.edu/Documents/in/Computer_Program?f_ri=15306"},{"id":321836,"name":"Spectrum","url":"https://www.academia.edu/Documents/in/Spectrum?f_ri=15306"},{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306"},{"id":335363,"name":"Far Infrared","url":"https://www.academia.edu/Documents/in/Far_Infrared?f_ri=15306"},{"id":390056,"name":"Fourier transform","url":"https://www.academia.edu/Documents/in/Fourier_transform?f_ri=15306"},{"id":671173,"name":"Atacama Large Millimeter Array","url":"https://www.academia.edu/Documents/in/Atacama_Large_Millimeter_Array?f_ri=15306"},{"id":898070,"name":"Experimental Measurement","url":"https://www.academia.edu/Documents/in/Experimental_Measurement?f_ri=15306"},{"id":1647408,"name":"Measurement Uncertainty","url":"https://www.academia.edu/Documents/in/Measurement_Uncertainty?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_14287882" data-work_id="14287882" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/14287882/Weeding_the_Cosmos_FIR_synchrotron_spectroscopy_of_methanol_at_the_Canadian_Light_Source">Weeding the Cosmos – FIR synchrotron spectroscopy of methanol at the Canadian Light Source</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/14287882" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="8d1b8007e3aa0153b2273e602b917fdd" rel="nofollow" data-download="{"attachment_id":44353962,"asset_id":14287882,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" 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class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/15001946/A_Herschel_PACS_and_SPIRE_study_of_the_dust_content_of_the_Cassiopeia_A_supernova_remnant">A Herschel PACS and SPIRE study of the dust content of the Cassiopeia A supernova remnant</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/15001946" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="c4c7b5facd239c7fd84a090c70bea2ad" rel="nofollow" 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Marchetti","profile_url":"https://independent.academia.edu/LMarchetti1?f_ri=15306","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":11050,"name":"Galaxy Formation and Evolution","url":"https://www.academia.edu/Documents/in/Galaxy_Formation_and_Evolution?f_ri=15306","nofollow":false},{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false},{"id":97563,"name":"Galaxy evolution","url":"https://www.academia.edu/Documents/in/Galaxy_evolution?f_ri=15306","nofollow":false},{"id":188982,"name":"High redshift galaxies and quasars","url":"https://www.academia.edu/Documents/in/High_redshift_galaxies_and_quasars?f_ri=15306","nofollow":false},{"id":335361,"name":"Infrared","url":"https://www.academia.edu/Documents/in/Infrared?f_ri=15306"},{"id":869493,"name":"Sloan Digital Sky Survey","url":"https://www.academia.edu/Documents/in/Sloan_Digital_Sky_Survey?f_ri=15306"},{"id":2217031,"name":"Spectral Energy Distribution","url":"https://www.academia.edu/Documents/in/Spectral_Energy_Distribution?f_ri=15306"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_21681224" data-work_id="21681224" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/21681224/A_chemical_inventory_of_the_S_type_AGB_star_%CF%87_Cygni_based_on_Herschel_HIFI_observations_of_circumstellar_line_emission">A chemical inventory of the S-type AGB star χ Cygni based on Herschel /HIFI observations of circumstellar line emission</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item 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href="https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_">Dust (Astronomy & Astrophysics)</a>, <script data-card-contents-for-ri="11125" type="text/json">{"id":11125,"name":"Dust (Astronomy \u0026 Astrophysics)","url":"https://www.academia.edu/Documents/in/Dust_Astronomy_and_Astrophysics_?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="15306" href="https://www.academia.edu/Documents/in/Herschel_Space_Observatory">Herschel Space Observatory</a>, <script data-card-contents-for-ri="15306" type="text/json">{"id":15306,"name":"Herschel Space Observatory","url":"https://www.academia.edu/Documents/in/Herschel_Space_Observatory?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="290733" href="https://www.academia.edu/Documents/in/Stars">Stars</a>, <script data-card-contents-for-ri="290733" type="text/json">{"id":290733,"name":"Stars","url":"https://www.academia.edu/Documents/in/Stars?f_ri=15306","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="442314" href="https://www.academia.edu/Documents/in/Radiative_Transfer">Radiative Transfer</a><script data-card-contents-for-ri="442314" type="text/json">{"id":442314,"name":"Radiative Transfer","url":"https://www.academia.edu/Documents/in/Radiative_Transfer?f_ri=15306","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=21681224]'), work: {"id":21681224,"title":"A chemical inventory of the S-type AGB star χ Cygni based on Herschel /HIFI observations of circumstellar line 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hidden" data-follow-ri-id="4363">Follow</a><a class="u-tcGray u-textDecorationNone u-linkUnstyled u-fw500 hidden" data-unfollow-ri-id="4363">Following</a></div></li><li class="list-group-item media_v2 u-mt0x u-p3x"><div class="media-body"><div class="u-tcGrayDarker u-fw700"><a class="u-tcGrayDarker" href="https://www.academia.edu/Documents/in/History_of_Islamic_Astronomy">History of Islamic Astronomy</a></div></div><div class="media-right media-middle"><a class="u-tcGreen u-textDecorationNone u-linkUnstyled u-fw500 hidden" data-follow-ri-id="30551">Follow</a><a class="u-tcGray u-textDecorationNone u-linkUnstyled u-fw500 hidden" data-unfollow-ri-id="30551">Following</a></div></li><li class="list-group-item media_v2 u-mt0x u-p3x"><div class="media-body"><div class="u-tcGrayDarker u-fw700"><a class="u-tcGrayDarker" href="https://www.academia.edu/Documents/in/Extragalactic_Astronomy">Extragalactic Astronomy</a></div></div><div class="media-right media-middle"><a class="u-tcGreen 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