<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Thompson SE</submitter><funding>UK Space Agency</funding><funding>Villum Fonden</funding><funding>European Research Council</funding><funding>Science Astrophysics NASA</funding><pagination>38</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC7477822</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>235(2)</volume><pubmed_abstract>We present the Kepler Object of Interest (KOI) catalog of transiting exoplanets based on searching four years of &lt;i>Kepler&lt;/i> time series photometry (Data Release 25, Q1-Q17). The catalog contains 8054 KOIs of which 4034 are planet candidates with periods between 0.25 and 632 days. Of these candidates, 219 are new in this catalog and include two new candidates in multi-planet systems (KOI-82.06 and KOI-2926.05), and ten new high-reliability, terrestrial-size, habitable zone candidates. This catalog was created using a tool called the Robovetter which automatically vets the DR25 Threshold Crossing Events (TCEs) found by the &lt;i>Kepler&lt;/i> Pipeline (Twicken et al. 2016). Because of this automation, we were also able to vet simulated data sets and therefore measure how well the Robovetter sep</pubmed_abstract><journal>The Astrophysical journal. Supplement series</journal><pubmed_title>PLANETARY CANDIDATES OBSERVED BY &lt;i>Kepler&lt;/i>. VIII. A FULLY AUTOMATED CATALOG WITH MEASURED COMPLETENESS AND RELIABILITY BASED ON DATA RELEASE 25.</pubmed_title><pmcid>PMC7477822</pmcid><funding_grant_id>ST/R003297/1</funding_grant_id><funding_grant_id>267864</funding_grant_id><funding_grant_id>00010118</funding_grant_id><pubmed_authors>Akeson R</pubmed_authors><pubmed_authors>Dupree AK</pubmed_authors><pubmed_authors>Barclay T</pubmed_authors><pubmed_authors>Haas MR</pubmed_authors><pubmed_authors>Ciardi DR</pubmed_authors><pubmed_authors>Shporer A</pubmed_authors><pubmed_authors>Cochran WD</pubmed_authors><pubmed_authors>Christiansen JL</pubmed_authors><pubmed_authors>Burke CJ</pubmed_authors><pubmed_authors>Lissauer JJ</pubmed_authors><pubmed_authors>Girouard FR</pubmed_authors><pubmed_authors>Isaacson H</pubmed_authors><pubmed_authors>Tenenbaum P</pubmed_authors><pubmed_authors>Barentsen G</pubmed_authors><pubmed_authors>Huber D</pubmed_authors><pubmed_authors>Koch DG</pubmed_authors><pubmed_authors>Seader SE</pubmed_authors><pubmed_authors>Li J</pubmed_authors><pubmed_authors>Geary JC</pubmed_authors><pubmed_authors>Still M</pubmed_authors><pubmed_authors>Latham DW</pubmed_authors><pubmed_authors>Jenkins JM</pubmed_authors><pubmed_authors>Clarke BD</pubmed_authors><pubmed_authors>Campbell JR</pubmed_authors><pubmed_authors>Morton TD</pubmed_authors><pubmed_authors>Batalha N</pubmed_authors><pubmed_authors>Quintana EV</pubmed_authors><pubmed_authors>Howell SB</pubmed_authors><pubmed_authors>Christensen-Dalsgaard J</pubmed_authors><pubmed_authors>Van Cleve JE</pubmed_authors><pubmed_authors>Bryson S</pubmed_authors><pubmed_authors>Mullally F</pubmed_authors><pubmed_authors>Ragozzine D</pubmed_authors><pubmed_authors>Wolfgang A</pubmed_authors><pubmed_authors>Ford EB</pubmed_authors><pubmed_authors>Catanzarite J</pubmed_authors><pubmed_authors>Dotson JL</pubmed_authors><pubmed_authors>Welsh WF</pubmed_authors><pubmed_authors>Coughlin JL</pubmed_authors><pubmed_authors>Caldwell DA</pubmed_authors><pubmed_authors>Charbonneau D</pubmed_authors><pubmed_authors>Borucki WJ</pubmed_authors><pubmed_authors>Smith JC</pubmed_authors><pubmed_authors>Dunham EW</pubmed_authors><pubmed_authors>Mathur S</pubmed_authors><pubmed_authors>Chaplin WJ</pubmed_authors><pubmed_authors>Henze CE</pubmed_authors><pubmed_authors>Zamudio KA</pubmed_authors><pubmed_authors>Steffen JH</pubmed_authors><pubmed_authors>Twicken JD</pubmed_authors><pubmed_authors>Hoffman K</pubmed_authors><pubmed_authors>Thompson SE</pubmed_authors><pubmed_authors>Morris RL</pubmed_authors><pubmed_authors>Prsa A</pubmed_authors><pubmed_authors>Aguirre VS</pubmed_authors><pubmed_authors>Rowe JF</pubmed_authors><pubmed_authors>Klaus TC</pubmed_authors><pubmed_authors>Ramirez SV</pubmed_authors><pubmed_authors>Wohler B</pubmed_authors><pubmed_authors>Kjeldsen H</pubmed_authors><pubmed_authors>Doyle L</pubmed_authors></additional><is_claimable>false</is_claimable><name>PLANETARY CANDIDATES OBSERVED BY &lt;i>Kepler&lt;/i>. VIII. A FULLY AUTOMATED CATALOG WITH MEASURED COMPLETENESS AND RELIABILITY BASED ON DATA RELEASE 25.</name><description>We present the Kepler Object of Interest (KOI) catalog of transiting exoplanets based on searching four years of &lt;i>Kepler&lt;/i> time series photometry (Data Release 25, Q1-Q17). The catalog contains 8054 KOIs of which 4034 are planet candidates with periods between 0.25 and 632 days. Of these candidates, 219 are new in this catalog and include two new candidates in multi-planet systems (KOI-82.06 and KOI-2926.05), and ten new high-reliability, terrestrial-size, habitable zone candidates. This catalog was created using a tool called the Robovetter which automatically vets the DR25 Threshold Crossing Events (TCEs) found by the &lt;i>Kepler&lt;/i> Pipeline (Twicken et al. 2016). Because of this automation, we were also able to vet simulated data sets and therefore measure how well the Robovetter sep</description><dates><release>2018-01-01T00:00:00Z</release><publication>2018 Apr</publication><modification>2025-04-18T11:24:48.427Z</modification><creation>2020-09-13T07:06:42Z</creation></dates><accession>S-EPMC7477822</accession><cross_references><pubmed>32908325</pubmed><doi>10.3847/1538-4365/aab4f9</doi></cross_references></HashMap>