PLANETARY CANDIDATES FROM THE FIRST YEAR OF THE K2 MISSION

被引：174

作者：

Vanderburg, Andrew ^{[1
]}

Latham, David W. ^{[1
]}

Buchhave, Lars A. ^{[2
,3
]}

Bieryla, Allyson ^{[1
]}

Berlind, Perry ^{[1
]}

Calkins, Michael L. ^{[1
]}

Esquerdo, Gilbert A. ^{[1
]}

Welsh, Sophie ^{[1
]}

Johnson, John Asher ^{[1
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[2] Univ Copenhagen, Nat Hist Museum Denmark, Ctr Star & Planet Format, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark

[3] Univ Copenhagen, Niels Bohr Inst, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2016年 / 222卷 / 01期

关键词：

methods: data analysis; planets and satellites: detection; techniques: photometric; TRANSIT SIGNAL RECOVERY; LIGHT CURVES; COLOR TRANSFORMATIONS; ECLIPSING BINARIES; INTRINSIC COLORS; BLEND SCENARIOS; KEPLER MISSION; MAIN-SEQUENCE; HOT JUPITERS; DATA RELEASE;

D O I：

10.3847/0067-0049/222/1/14

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Kepler Space Telescope is currently searching for planets transiting stars along the ecliptic plane as part of its extended K2 mission. We processed the publicly released data from the first year of K2 observations (Campaigns 0, 1, 2, and 3) and searched for periodic eclipse signals consistent with planetary transits. Out of the 59,174 targets that we searched, we detect 234 planetary candidates around 208 stars. These candidates range in size from gas giants to smaller than the Earth, and range in orbital periods from hours to over a month. We conducted initial reconnaissance spectroscopy of 68 of the brighter candidate host stars, and present high-resolution optical spectra for these stars. We make all of our data products, including light curves, spectra, and vetting diagnostics available to users online.

引用

页数：15

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