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• W3105223721 abstract "&lt;p class=&quot;p1&quot;&gt;&lt;span class=&quot;s1&quot;&gt;The Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;spacecraft was reactivated in December 2013 and since then has been &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;conducting an all-sky survey at 3.4 and 4.6 microns to discover and &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;characterize asteroids and comets that come close to the Earth.&amp;#160; &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;NEOWISE employs an automated pipeline for the detection of moving &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;objects, recording their astrometry and photometry and reporting &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;positions to the Minor Planet Center for archiving.&lt;span class=&quot;Apple-converted-space&quot;&gt;&amp;#160; &lt;/span&gt;However, there &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;are a subset of near-Earth objects that are not found by the automated &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;system due to rates of motion or acceleration outside the pipeline &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;limits, an insufficient number of detections, or confusion with &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;background sources.&lt;span class=&quot;Apple-converted-space&quot;&gt;&amp;#160; &lt;/span&gt;Because NEOWISE archives every full-frame image &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;obtained during the survey, detections of these objects can be &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;recovered by manually searching the expected positions for coincident &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;sources.&lt;/span&gt;&lt;/p&gt; &lt;p class=&quot;p1&quot;&gt;&lt;span class=&quot;s1&quot;&gt;We have performed searches for near-Earth objects in the NEOWISE &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;archives from 2013 to 2019, recovering detections for over 400 objects &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;and enabling fitting of their diameters and albedos (Masiero et &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;al. 2018, Masiero et al. 2020).&lt;span class=&quot;Apple-converted-space&quot;&gt;&amp;#160; &lt;/span&gt;This builds on earlier work that &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;searched the data from the cryogenic phase of the original WISE &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;mission (Mainzer et al. 2014).&lt;span class=&quot;Apple-converted-space&quot;&gt;&amp;#160; &lt;/span&gt;Objects found through this technique &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;tend to be smaller than those detected by the automated processing. &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;The distribution of albedos for these objects is skewed to high &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;reflectivities, as is expected for a population that is &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;optically-selected.&lt;/span&gt;&lt;/p&gt; &lt;p class=&quot;p1&quot;&gt;&lt;span class=&quot;s1&quot;&gt;Here we present the results of our searches along with the physical &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;properties of the recovered objects.&lt;span class=&quot;Apple-converted-space&quot;&gt;&amp;#160; &lt;/span&gt;We also will discuss the reasons &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;these objects were missed by the automated processing, and what the &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;observed physical property distribution implies about any remaining &lt;/span&gt;&lt;span class=&quot;s1&quot;&gt;objects still waiting to be found in the data.&lt;/span&gt;&lt;/p&gt;" @default.
• W3105223721 created "2020-11-23" @default.
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• W3105223721 date "2020-10-08" @default.
• W3105223721 modified "2023-09-27" @default.
• W3105223721 title "Physical properties of near-Earth asteroids manually recovered from NEOWISE data" @default.
• W3105223721 doi "https://doi.org/10.5194/epsc2020-333" @default.
• W3105223721 hasPublicationYear "2020" @default.
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