REVISED STELLAR PROPERTIES OF KEPLER TARGETS FOR THE QUARTER 1-16 TRANSIT DETECTION RUN

被引：387

作者：

Huber, Daniel ^{[1
,2
]}

Aguirre, Victor Silva ^{[3
]}

Matthews, Jaymie M. ^{[4
]}

Pinsonneault, Marc H. ^{[5
]}

Gaidos, Eric ^{[6
]}

Garcia, Rafael A. ^{[7
]}

Hekker, Saskia ^{[8
,9
]}

Mathur, Savita ^{[10
]}

Mosser, Benoit ^{[11
]}

Torres, Guillermo ^{[12
]}

Bastien, Fabienne A. ^{[13
]}

Basu, Sarbani ^{[14
]}

Bedding, Timothy R. ^{[3
,15
]}

Chaplin, William J. ^{[3
,16
]}

Demory, Brice-Olivier ^{[17
]}

Fleming, Scott W. ^{[18
]}

Guo, Zhao ^{[19
]}

Mann, Andrew W. ^{[20
]}

Rowe, Jason F. ^{[1
,2
]}

Serenelli, Aldo M. ^{[21
]}

Smith, Myron A. ^{[22
]}

Stello, Dennis ^{[3
,15
]}

机构：

[1] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA

[2] SETI Inst, Mountain View, CA 94043 USA

[3] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, DK-8000 Aarhus C, Denmark

[4] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada

[5] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA

[6] Univ Hawaii Manoa, Dept Geol & Geophys, Honolulu, HI 96822 USA

[7] Univ Paris 07, IRFU SAp, Ctr Saclay, Lab AIM,CEA DSM CNRS, F-91191 Gif Sur Yvette, France

[8] Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany

[9] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 XH Amsterdam, Netherlands

[10] Space Sci Inst, Boulder, CO 80301 USA

[11] Univ Paris 06, Univ Denis, Observ Paris, LESIA,CNRS, F-92195 Meudon, France

[12] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[13] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA

[14] Yale Univ, Dept Astron, New Haven, CT 06511 USA

[15] Univ Sydney, Sch Phys, Sydney Inst Astron SIfA, Sydney, NSW 2006, Australia

[16] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[17] MIT, Dept Phys, Cambridge, MA 02139 USA

[18] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[19] Georgia State Univ, Ctr High Angular Resolut Astron, Atlanta, GA 30302 USA

[20] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA

[21] Inst Ciencias Espacio CSIC IEEC, Fac Ciencias, E-08193 Bellaterra, Spain

[22] Natl Opt Astron Observ, Tucson, AZ 85719 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2014年 / 211卷 / 01期

基金：

新加坡国家研究基金会; 美国国家航空航天局; 美国国家科学基金会; 欧洲研究理事会; 英国科学技术设施理事会;

关键词：

catalogs; planetary systems; stars: fundamental parameters; stars: oscillations; techniques: photometric; SOLAR-LIKE OSCILLATIONS; R-CIRCLE-PLUS; MULTIPLE-PLANET SYSTEMS; LOW-MASS STARS; 1ST; MONTHS; RED-GIANT; HABITABLE-ZONE; HOT-JUPITER; ATMOSPHERIC PARAMETERS; SOPHIE VELOCIMETRY;

D O I：

10.1088/0067-0049/211/1/2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present revised properties for 196,468 stars observed by the NASA Kepler mission and used in the analysis of Quarter 1-16 (Q1-Q16) data to detect and characterize transiting planets. The catalog is based on a compilation of literature values for atmospheric properties (temperature, surface gravity, and metallicity) derived from different observational techniques (photometry, spectroscopy, asteroseismology, and exoplanet transits), which were then homogeneously fitted to a grid of Dartmouth stellar isochrones. We use broadband photometry and asteroseismology to characterize 11,532 Kepler targets which were previously unclassified in the Kepler Input Catalog (KIC). We report the detection of oscillations in 2762 of these targets, classifying them as giant stars and increasing the number of known oscillating giant stars observed by Kepler by similar to 20% to a total of similar to 15,500 stars. Typical uncertainties in derived radii and masses are similar to 40% and similar to 20%, respectively, for stars with photometric constraints only, and 5%-15% and similar to 10% for stars based on spectroscopy and/or asteroseismology, although these uncertainties vary strongly with spectral type and luminosity class. A comparison with the Q1-Q12 catalog shows a systematic decrease in radii of M dwarfs, while radii for K dwarfs decrease or increase depending on the Q1-Q12 provenance (KIC or Yonsei-Yale isochrones). Radii of F-G dwarfs are on average unchanged, with the exception of newly identified giants. The Q1-Q16 star properties catalog is a first step toward an improved characterization of all Kepler targets to support planet-occurrence studies.

引用

页数：18

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