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CCD Astrometry of ``Critical List'' Minor Planets - NASA/ADS

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Telescope operation is completely automatic and is monitored remotely by an observer using another telescope at the station. On a typical night, 80 to 100 objects are observed. Positions are determined with respect to the Guide Star Catalog (GSC) stars appearing in each frame, and are generally accurate to +/-0.3 arcseconds. All results are published, usually within a few weeks after observation, in the Minor Planet Center (MPC) circulars. When this project began in March 1994, the plan was to do follow--on astrometry of recently--discovered near--Earth objects (NEOs). But the capacity of this observing program far exceeds the number of available NEOs. So the observing list was expanded to include several other categories of objects and projects, including minor planets of particular scientific interest, mass--determination candidates, objects which can be used to improved the dynamical reference frame, and MPC ``Critical List&#39;&#39; objects --- minor planets whose orbits and positions are especially in need of improvement. This paper will report on the progress to date in this last category of observation, on the quality of the results, and on some of the science being done or planned for the near future."> <!-- Open Graph --> <meta property="og:type" content="abstract"> <meta property="og:title" content="CCD Astrometry of ``Critical List&#39;&#39; Minor Planets"> <meta property="og:site_name" content="NASA/ADS"> <meta property="og:description" content="Minor planet observations are being made at the USNO Flagstaff Station with an 8-inch transit telescope with a CCD camera operated in scan mode. Telescope operation is completely automatic and is monitored remotely by an observer using another telescope at the station. On a typical night, 80 to 100 objects are observed. Positions are determined with respect to the Guide Star Catalog (GSC) stars appearing in each frame, and are generally accurate to +/-0.3 arcseconds. All results are published, usually within a few weeks after observation, in the Minor Planet Center (MPC) circulars. When this project began in March 1994, the plan was to do follow--on astrometry of recently--discovered near--Earth objects (NEOs). But the capacity of this observing program far exceeds the number of available NEOs. So the observing list was expanded to include several other categories of objects and projects, including minor planets of particular scientific interest, mass--determination candidates, objects which can be used to improved the dynamical reference frame, and MPC ``Critical List&#39;&#39; objects --- minor planets whose orbits and positions are especially in need of improvement. This paper will report on the progress to date in this last category of observation, on the quality of the results, and on some of the science being done or planned for the near future."> <meta property="og:url" content="https://ui.adsabs.harvard.edu/abs/1994AAS...185.4311M/abstract"> <meta property="og:image" content="https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg"> <meta property="article:published_time" content="12/1994"> <meta property="article:author" content="Monet, A. K. 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So the observing list was expanded to include several other categories of objects and projects, including minor planets of particular scientific interest, mass--determination candidates, objects which can be used to improved the dynamical reference frame, and MPC ``Critical List&#39;&#39; objects --- minor planets whose orbits and positions are especially in need of improvement. 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K. B.</a> </li> </ul> </div> <div class="s-abstract-text"> <h4 class="sr-only">Abstract</h4> <p> Minor planet observations are being made at the USNO Flagstaff Station with an 8-inch transit telescope with a CCD camera operated in scan mode. Telescope operation is completely automatic and is monitored remotely by an observer using another telescope at the station. On a typical night, 80 to 100 objects are observed. Positions are determined with respect to the Guide Star Catalog (GSC) stars appearing in each frame, and are generally accurate to +/-0.3 arcseconds. All results are published, usually within a few weeks after observation, in the Minor Planet Center (MPC) circulars. When this project began in March 1994, the plan was to do follow--on astrometry of recently--discovered near--Earth objects (NEOs). But the capacity of this observing program far exceeds the number of available NEOs. So the observing list was expanded to include several other categories of objects and projects, including minor planets of particular scientific interest, mass--determination candidates, objects which can be used to improved the dynamical reference frame, and MPC ``Critical List'' objects --- minor planets whose orbits and positions are especially in need of improvement. This paper will report on the progress to date in this last category of observation, on the quality of the results, and on some of the science being done or planned for the near future. </p> </div> <br> <dl class="s-abstract-dl-horizontal"> <dt>Publication:</dt> <dd> <div id="article-publication">American Astronomical Society Meeting Abstracts</div> </dd> <dt>Pub Date:</dt> <dd>December 1994</dd> <dt>Bibcode:</dt> <dd> <a href="/abs/1994AAS...185.4311M/abstract"> 1994AAS...185.4311M </a> <i class="icon-help" title="The bibcode is assigned by the ADS as a unique identifier for the paper."></i> </dd> </dl> </article> </div> <div data-widget="ShowCitations"></div> <div data-widget="ShowReferences"></div> <div data-widget="ShowCoreads"></div> <div data-widget="ShowSimilar"></div> <div data-widget="ShowTableofcontents"></div> <div data-widget="ShowGraphics"></div> <div data-widget="ShowExportcitation" data-origin="abstract"></div> <div data-widget="ShowMetrics" data-allow-redirect="false"></div> <div data-widget="MetaTagsWidget"></div> </div> </div> </div> <div class="s-right-col-container col-xs-12 col-sm-12 col-md-3 col-lg-2 s-right-column" id="right-col-container" > <div data-widget="ShowResources"> <div data-reactroot="" class="s-right-col-widget-container" style="padding: 10px" > <h3 class="s-right-col-widget-title">No Sources Found</h3> <div> <div class="resources__container"> </div> <div data-widget="ShowAssociated"> </div> </div> </div> </div> <div data-widget="ShowGraphicsSidebar"> </div> </div> </div> </div> </div> </div> </div> <div id="footer-container"> <div data-widget="FooterWidget"> <div class="footer s-footer"> <footer> <div class="__footer_wrapper"> <div class="__footer_brand"> 漏 The SAO/NASA Astrophysics Data System <div class="__footer_brand_extra"> <p> <i class="fa fa-envelope"></i> adshelp[at]cfa.harvard.edu </p> <p> The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement <em>NNX16AC86A</em> </p> </div> <div class="__footer_brand_logos"> <a href="http://www.nasa.gov" target="_blank" rel="noopener"> <img src="/styles/img/nasa.svg" alt="NASA logo" id="nasa-logo"> </a> <a href="http://www.si.edu" target="_blank" rel="noopener"> <img id="smithsonian-logo" src="/styles/img/smithsonian.svg" alt="Smithsonian logo"> </a> <a href="https://www.cfa.harvard.edu/" target="_blank" rel="noopener"> <img src="/styles/img/cfa.png" title="Harvard Center for Astrophysics logo" id="cfa-logo"> </a> </div> </div> <div class="__footer_list"> <div class="__footer_list_title"> Resources </div> <ul class="__footer_links"> <li> <a href="/about/" target="_blank" rel="noopener"> <i class="fa fa-question-circle"></i> About ADS </a> </li> <li> <a href="//ui.adsabs.harvard.edu/help/" target="_blank" rel="noopener"> <i class="fa fa-info-circle"></i> ADS Help </a> </li> <li> <a href="//ui.adsabs.harvard.edu/help/whats_new/" target="_blank" rel="noopener"> <i class="fa fa-bullhorn"></i> What's New </a> </li> <li> <a href="/about/careers/" target="_blank" rel="noopener"> <i class="fa fa-group"></i> Careers@ADS </a> </li> </ul> </div> <div class="__footer_list"> <div class="__footer_list_title"> Social </div> <ul class="__footer_links"> <li> <a href="//twitter.com/adsabs" target="_blank" rel="noopener"> <i class="fa fa-twitter"></i> @adsabs </a> </li> <li> <a href="//ui.adsabs.harvard.edu/blog/" target="_blank" rel="noopener"> <i class="fa fa-newspaper-o"></i> ADS Blog </a> </li> </ul> </div> <div class="__footer_list"> <div class="__footer_list_title"> Project </div> <ul class="__footer_links"> <li> <a href="/core/never">Switch to full ADS</a> </li> <li> <a href="https://adsisdownorjustme.herokuapp.com/" target="_blank" rel="noopener">Is ADS down? 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// initiate the autocomplete function on the "q" element, and pass along the operators array as possible autocomplete values: inputBox = document.getElementById("q") if (inputBox) { inputBox.focus() // autofucs inputBox.setSelectionRange(inputBox.value.length, inputBox.value.length); // bring cursor to the end autocomplete(inputBox, autoList); } </script> <script> (function() { // turn off no-js if we have javascript document.documentElement.className = document.documentElement.className.replace("no-js", "js"); function getCookie(cname) { var name = cname + "="; var decodedCookie = decodeURIComponent(document.cookie); var ca = decodedCookie.split(';'); for (var i = 0; i < ca.length; i++) { var c = ca[i]; while (c.charAt(0) == ' ') { c = c.substring(1); } if (c.indexOf(name) == 0) { return c.substring(name.length, c.length); } } return ""; } (function() { // looks for the cookie, and sets true if its 'always' const coreCookie = getCookie('core') === 'always'; // only load bumblebee if we detect the core cookie and we are on abstract page if (coreCookie || (!(/^\/abs\//.test(document.location.pathname)) && !coreCookie)) { return; 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