197 CANDIDATES AND 104 VALIDATED PLANETS IN <i>K2</i>'s FIRST FIVE FIELDS
dc.contributor.author | Crossfield, Ian J. M. | |
dc.contributor.author | Ciardi, David R. | |
dc.contributor.author | Petigura, Erik A. | |
dc.contributor.author | Sinukoff, Evan | |
dc.contributor.author | Schlieder, Joshua E. | |
dc.contributor.author | Howard, Andrew W. | |
dc.contributor.author | Beichman, Charles A. | |
dc.contributor.author | Isaacson, Howard | |
dc.contributor.author | Dressing, Courtney D. | |
dc.contributor.author | Christiansen, Jessie L. | |
dc.contributor.author | Fulton, Benjamin J. | |
dc.contributor.author | Lepine, Sebastien | |
dc.contributor.author | Weiss, Lauren | |
dc.contributor.author | Hirsch, Lea | |
dc.contributor.author | Livingston, John | |
dc.contributor.author | Baranec, Christoph | |
dc.contributor.author | Law, Nicholas M. | |
dc.contributor.author | Riddle, Reed | |
dc.contributor.author | Ziegler, Carl | |
dc.contributor.author | Howell, Steve B. | |
dc.contributor.author | Horch, Elliott | |
dc.contributor.author | Everett, Mark | |
dc.contributor.author | Teske, Johanna | |
dc.contributor.author | Martinez, Arturo O. | |
dc.contributor.author | Obermeier, Christian | |
dc.contributor.author | Benneke, Bjorn | |
dc.contributor.author | Scott, Nic | |
dc.contributor.author | Deacon, Niall | |
dc.contributor.author | Aller, Kimberly M. | |
dc.contributor.author | Hansen, Brad M. S. | |
dc.contributor.author | Mancini, Luigi | |
dc.contributor.author | Ciceri, Simona | |
dc.contributor.author | Brahm, Rafael | |
dc.contributor.author | Jordan, Andres | |
dc.contributor.author | Knutson, Heather A. | |
dc.contributor.author | Henning, Thomas | |
dc.contributor.author | Bonnefoy, Michael | |
dc.contributor.author | Liu, Michael C. | |
dc.contributor.author | Crepp, Justin R. | |
dc.contributor.author | Lothringer, Joshua | |
dc.contributor.author | Hinz, Phil | |
dc.contributor.author | Bailey, Vanessa | |
dc.contributor.author | Skemer, Andrew | |
dc.contributor.author | Defrere, Denis | |
dc.date.accessioned | 2025-01-23T21:29:30Z | |
dc.date.available | 2025-01-23T21:29:30Z | |
dc.date.issued | 2016 | |
dc.description.abstract | We present 197 planet candidates discovered using data from the first year of the NASA K2 mission (Campaigns 0-4), along with the results of an intensive program of photometric analyses, stellar spectroscopy, high-resolution imaging, and statistical validation. We distill these candidates into sets of 104 validated planets (57 in multi-planet systems), 30 false positives, and 63 remaining candidates. Our validated systems span a range of properties, with median values of R-P = 2.3 R-circle plus, P = 8.6 days, T-eff = 5300 K, and Kp = 12.7 mag. Stellar spectroscopy provides precise stellar and planetary parameters for most of these systems. We show that K2 has increased by 30% the number of small planets known to orbit moderately bright stars (1-4 R-circle plus, Kp = 9-13. mag). Of particular interest are 76 planets smaller than 2 R-circle plus, 15 orbiting stars brighter than Kp = 11.5. mag, 5 receiving Earth-like irradiation levels, and several multi-planet systems-including 4 planets orbiting the M dwarf K2-72 near mean-motion resonances. By quantifying the likelihood that each candidate is a planet we demonstrate that our candidate sample has an overall false positive rate of 15%-30%, with rates substantially lower for small candidates (<2 R-circle plus) and larger for candidates with radii >8 R-circle plus and/or with P < 3 days. Extrapolation of the current planetary yield suggests that K2 will discover between 500 and 1000 planets in its planned four-year mission, assuming sufficient follow-up resources are available. Efficient observing and analysis, together with an organized and coherent follow-up strategy, are essential for maximizing the efficacy of planet-validation efforts for K2, TESS, and future large-scale surveys. | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.3847/0067-0049/226/1/7 | |
dc.identifier.eissn | 1538-4365 | |
dc.identifier.issn | 0067-0049 | |
dc.identifier.uri | https://doi.org/10.3847/0067-0049/226/1/7 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/101433 | |
dc.identifier.wosid | WOS:000400516900003 | |
dc.issue.numero | 1 | |
dc.language.iso | en | |
dc.revista | Astrophysical journal supplement series | |
dc.rights | acceso restringido | |
dc.subject | catalogs | |
dc.subject | planets and satellites: fundamental parameters | |
dc.subject | planets and satellites: general | |
dc.subject | techniques: high angular resolution | |
dc.subject | techniques: photometric | |
dc.subject | techniques: spectroscopic | |
dc.subject.ods | 13 Climate Action | |
dc.subject.odspa | 13 Acción por el clima | |
dc.title | 197 CANDIDATES AND 104 VALIDATED PLANETS IN <i>K2</i>'s FIRST FIVE FIELDS | |
dc.type | artículo | |
dc.volumen | 226 | |
sipa.index | WOS | |
sipa.trazabilidad | WOS;2025-01-12 |