{"id":26,"date":"2024-05-13T17:10:00","date_gmt":"2024-05-13T17:10:00","guid":{"rendered":"https:\/\/dev.neos.epss.ucla.edu\/?p=26"},"modified":"2025-09-10T21:06:13","modified_gmt":"2025-09-10T21:06:13","slug":"science-data-processing","status":"publish","type":"post","link":"https:\/\/neos.epss.ucla.edu\/index.php\/2024\/05\/13\/science-data-processing\/","title":{"rendered":"Science Data Processing"},"content":{"rendered":"\n<p class=\"has-small-font-size\">The NEO Surveyor science data processing pipeline builds our team&#8217;s experience with discovering asteroids using a space-based infrared telescope, WISE. Our team developed software that discovered new\u00a0asteroids and comets in near real-time; the asteroid-hunting portion of the WISE project is known as NEOWISE.\u00a0<br><br>The NEOWISE software developed by our team allowed us to detect more than 158,000 asteroids and comets (including about 34,000 new discoveries) with heat-sensitive infrared images. These included 577 NEOs (135 of which were new discoveries credited to NEOWISE).<br><br>We will adapt the existing NEOWISE science data processing to work with NEO Surveyor&#8217;s images, allowing us to distinguish moving asteroids and comets from background stars and galaxies.\u00a0 NEO Surveyor&#8217;s survey cadence is optimized to allow the mission to not only discover new asteroids, but to observe them enough times to ensure that they can be found again.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The NEO Surveyor science data processing pipeline builds our team&#8217;s experience with discovering asteroids using a space-based infrared telescope, WISE. Our team developed software that discovered new\u00a0asteroids and comets in near real-time; the asteroid-hunting portion of the WISE project is known as NEOWISE.\u00a0 The NEOWISE software developed by our team allowed us to detect more [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-26","post","type-post","status-publish","format-standard","hentry","category-uncategorized"],"_links":{"self":[{"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/posts\/26","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/comments?post=26"}],"version-history":[{"count":3,"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/posts\/26\/revisions"}],"predecessor-version":[{"id":136,"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/posts\/26\/revisions\/136"}],"wp:attachment":[{"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/media?parent=26"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/categories?post=26"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/neos.epss.ucla.edu\/index.php\/wp-json\/wp\/v2\/tags?post=26"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}