A TESS Dress Rehearsal: Planetary Candidates and Variables from K2 Campaign 17
العنوان: | A TESS Dress Rehearsal: Planetary Candidates and Variables from K2 Campaign 17 |
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المؤلفون: | Martin Owens, Lizhou Sha, Elisabeth R. Newton, Avi Shporer, Adina D. Feinstein, David W. Latham, Chelsea X. Huang, Zhuchang Zhan, Jennifer Burt, Isabel Kain, Liang Yu, Trevor J. David, Merrin Peterson, Perry Berlind, Zahra Essack, David Berardo, Michael L. Calkins, Erik A. Petigura, Courtney D. Dressing, Megan Bedell, Sarah Ballard, Allyson Bieryla, Benjamin J. Fulton, Jason Dittmann, José Vinícius de Miranda Cardoso, Karen A. Collins, Andrew W. Howard, David R. Ciardi, Jessie L. Christiansen, Gilbert A. Esquerdo, Nicholas Mehrle, Samuel N. Quinn, Sara Seager, Joshua E. Schlieder, Natalia Guerrero, John H. Livingston, Björn Benneke, Howard Isaacson, Joseph E. Rodriguez, Makennah Bristow, Erica J. Gonzales, M. R. Kosiarek, Ian J. M. Crossfield |
سنة النشر: | 2018 |
مصطلحات موضوعية: | Physics, Earth and Planetary Astrophysics (astro-ph.EP), 010504 meteorology & atmospheric sciences, Astronomy, FOS: Physical sciences, Astronomy and Astrophysics, Light curve, 01 natural sciences, Exoplanet, Stars, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Planet, 0103 physical sciences, 010303 astronomy & astrophysics, Data release, Solar and Stellar Astrophysics (astro-ph.SR), 0105 earth and related environmental sciences, Astrophysics - Earth and Planetary Astrophysics |
الوصف: | We produce light curves for all ~34,000 targets observed with K2 in Campaign 17 (C17), identifying 34 planet candidates, 184 eclipsing binaries, and 222 other periodic variables. The location of the C17 field means follow-up can begin immediately now that the campaign has concluded and interesting targets have been identified. The C17 field has a large overlap with C6, so this latest campaign also offers a rare opportunity to study a large number of targets already observed in a previous K2 campaign. The timing of the C17 data release, shortly before science operations begin with the Transiting Exoplanet Survey Satellite (TESS), also lets us exercise some of the tools and methods developed for identification and dissemination of planet candidates from TESS. We find excellent agreement between these results and those identified using only K2-based tools. Among our planet candidates are several planet candidates with sizes < 4 R_E and orbiting stars with KepMag < 10 (indicating good RV targets of the sort TESS hopes to find) and a Jupiter-sized single-transit event around a star already hosting a 6 d planet candidate. Submitted. 19 pages, 5 figures, 5 tables, 34 planet candidates, 184 EBs, 34,000 lightcurves |
وصف الملف: | application/pdf |
اللغة: | English |
URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e135a7af762174e7358c1a477f0be49 http://arxiv.org/abs/1806.03127 |
حقوق: | OPEN |
رقم الأكسشن: | edsair.doi.dedup.....9e135a7af762174e7358c1a477f0be49 |
قاعدة البيانات: | OpenAIRE |
الوصف غير متاح. |