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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00005107naa a2200889 4500
001oai:DiVA.org:su-143871
003SwePub
008170602s2016 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1438712 URI
024a https://doi.org/10.3847/0067-0049/226/1/72 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Crossfield, Ian J. M.4 aut
2451 0a 197 CANDIDATES AND 104 VALIDATED PLANETS IN K2's FIRST FIVE FIELDS
264 c 2016-09-02
264 1b American Astronomical Society,c 2016
338 a print2 rdacarrier
520 a 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.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a catalogs
653 a planets and satellites: fundamental parameters
653 a planets and satellites: general
653 a techniques: high angular resolution
653 a techniques: photometric
653 a techniques: spectroscopic
700a Ciardi, David R.4 aut
700a Petigura, Erik A.4 aut
700a Sinukoff, Evan4 aut
700a Schlieder, Joshua E.4 aut
700a Howard, Andrew W.4 aut
700a Beichman, Charles A.4 aut
700a Isaacson, Howard4 aut
700a Dressing, Courtney D.4 aut
700a Christiansen, Jessie L.4 aut
700a Fulton, Benjamin J.4 aut
700a Lepine, Sebastien4 aut
700a Weiss, Lauren4 aut
700a Hirsch, Lea4 aut
700a Livingston, John4 aut
700a Baranec, Christoph4 aut
700a Law, Nicholas M.4 aut
700a Riddle, Reed4 aut
700a Ziegler, Carl4 aut
700a Howell, Steve B.4 aut
700a Horch, Elliott4 aut
700a Everett, Mark4 aut
700a Teske, Johanna4 aut
700a Martinez, Arturo O.4 aut
700a Obermeier, Christian4 aut
700a Benneke, Björn4 aut
700a Scott, Nic4 aut
700a Deacon, Niall4 aut
700a Aller, Kimberly M.4 aut
700a Hansen, Brad M. S.4 aut
700a Mancini, Luigi4 aut
700a Ciceri, Simonau Stockholms universitet,Institutionen för astronomi,Max Planck Institut für Astronomie, Germany4 aut0 (Swepub:su)scice
700a Brahm, Rafael4 aut
700a Jordan, Andres4 aut
700a Knutson, Heather A.4 aut
700a Henning, Thomas4 aut
700a Bonnefoy, Michael4 aut
700a Liu, Michael C.4 aut
700a Crepp, Justin R.4 aut
700a Lothringer, Joshua4 aut
700a Hinz, Phil4 aut
700a Bailey, Vanessa4 aut
700a Skemer, Andrew4 aut
700a Defrere, Denis4 aut
710a Stockholms universitetb Institutionen för astronomi4 org
773t Astrophysical Journal Supplement Seriesd : American Astronomical Societyg 226:1q 226:1x 0067-0049x 1538-4365
856u https://repository.arizona.edu/bitstream/10150/624074/1/Crossfield_2016_ApJS_226_7.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-143871
8564 8u https://doi.org/10.3847/0067-0049/226/1/7

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