197 CANDIDATES AND 104 VALIDATED PLANETS IN K2's FIRST FIVE FIELDS

被引:156
作者
Crossfield, Ian J. M. [1 ,29 ]
Ciardi, David R. [2 ]
Petigura, Erik A. [3 ]
Sinukoff, Evan [4 ]
Schlieder, Joshua E. [2 ,5 ]
Howard, Andrew W. [4 ]
Beichman, Charles A. [2 ]
Isaacson, Howard [6 ]
Dressing, Courtney D. [3 ]
Christiansen, Jessie L. [2 ]
Fulton, Benjamin J. [4 ]
Lepine, Sebastien [7 ]
Weiss, Lauren [6 ]
Hirsch, Lea [6 ]
Livingston, John [8 ]
Baranec, Christoph [9 ]
Law, Nicholas M. [10 ]
Riddle, Reed [11 ]
Ziegler, Carl [10 ]
Howell, Steve B.
Horch, Elliott [12 ]
Everett, Mark [13 ]
Teske, Johanna [14 ]
Martinez, Arturo O. [7 ,15 ]
Obermeier, Christian [16 ]
Benneke, Bjorn [3 ]
Scott, Nic [17 ]
Deacon, Niall [18 ]
Aller, Kimberly M. [4 ]
Hansen, Brad M. S. [19 ,20 ]
Mancini, Luigi [16 ]
Ciceri, Simona [16 ,21 ]
Brahm, Rafael [22 ]
Jordan, Andres [22 ,23 ]
Knutson, Heather A. [3 ]
Henning, Thomas [16 ]
Bonnefoy, Michael [24 ,25 ]
Liu, Michael C. [4 ]
Crepp, Justin R. [26 ]
Lothringer, Joshua [1 ]
Hinz, Phil
Bailey, Vanessa [27 ]
Skemer, Andrew [27 ,28 ,29 ]
Defrere, Denis [24 ,25 ,30 ]
机构
[1] Univ Arizona, Lunar & Planetary Lab, 1629 E Univ Blvd, Tucson, AZ 85721 USA
[2] NASA, CALTECH, Exoplanet Sci Inst, Pasadena, CA USA
[3] CALTECH, Geol & Planetary Sci, Pasadena, CA 91125 USA
[4] Univ Hawaii Manoa, Inst Astron, Honolulu, HI 96822 USA
[5] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[6] Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA
[7] Georgia State Univ, Dept Phys & Astron, Atlanta, GA 30303 USA
[8] Univ Tokyo, Dept Astron, Bunkyo Ku, 7-3-1, Tokyo 1130033, Japan
[9] Univ Hawaii Manoa, Inst Astron, Hilo, HI USA
[10] Univ North Carolina Chapel Hill, Dept Phys & Astron, Chapel Hill, NC USA
[11] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA
[12] Southern Connecticut State Univ, Dept Phys, New Haven, CT USA
[13] Natl Opt Astron Observ, Tucson, AZ 85726 USA
[14] Carnegie Dept Terr Magnetism, Washington, DC USA
[15] San Diego State Univ, Dept Astron, San Diego, CA 92182 USA
[16] Max Planck Inst Astron, Heidelberg, Germany
[17] Univ Sydney, Sydney Inst Astron, Redfern, Australia
[18] Univ Hertfordshire, Ctr Astrophys Res, Hatfield, Herts, England
[19] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA USA
[20] Univ Calif Los Angeles, Inst Geophys & Planetary Sci, Los Angeles, CA 90024 USA
[21] Stockholm Univ, Dept Astron, SE-10691 Stockholm, Sweden
[22] Millennium Inst Astrophys, Av Vicuna Mackenna 4860, Santiago 7820436, Chile
[23] Pontificia Univ Catolica Chile, Fac Fis, Inst Astrofis, Av Vicuna Mackenna 4860, Santiago 7820436, Chile
[24] Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France
[25] CNRS, IPAG, F-38000 Grenoble, France
[26] Univ Notre Dame, Dept Phys, 225 Nieuwland Sci Hall, Notre Dame, IN 46556 USA
[27] Univ Arizona, Steward Observ, Tucson, AZ USA
[28] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
[29] Univ Calif Santa Cruz, Dept Astron, Santa Cruz, CA 95064 USA
[30] Univ Liege, Dept Astrophys Geophys & Oceanog, B-4000 Cointe Ougree, Belgium
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
catalogs; planets and satellites: fundamental parameters; planets and satellites: general; techniques: high angular resolution; techniques: photometric; techniques: spectroscopic; EARTH-SIZE PLANETS; ADAPTIVE OPTICS; HOT JUPITER; TRANSIT CANDIDATES; ECLIPSING BINARIES; KEPLER OBJECTS; SUPER-EARTH; M DWARFS; BLEND SCENARIOS; PAN-STARRS;
D O I
10.3847/0067-0049/226/1/7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
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页数:20
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