Preparation of Kepler light curves for asteroseismic analyses

被引:234
作者
Garcia, R. A. [1 ]
Hekker, S. [2 ,3 ]
Stello, D. [4 ]
Gutierrez-Soto, J. [5 ]
Handberg, R. [6 ]
Huber, D. [4 ]
Karoff, C. [6 ]
Uytterhoeven, K. [1 ]
Appourchaux, T. [7 ]
Chaplin, W. J. [3 ]
Elsworth, Y. [3 ]
Mathur, S. [8 ]
Ballot, J. [9 ]
Christensen-Dalsgaard, J. [6 ]
Gilliland, R. L. [10 ]
Houdek, G. [11 ]
Jenkins, J. M. [12 ]
Kjeldsen, H. [6 ]
McCauliff, S. [13 ]
Metcalfe, T. [8 ]
Middour, C. K. [13 ]
Molenda-Zakowicz, J. [14 ]
Monteiro, M. J. P. F. G. [15 ]
Smith, J. C. [12 ]
Thompson, M. J. [8 ]
机构
[1] Univ Paris Diderot, Lab AIM, CEA DSM, Ctr Saclay,IRFU SAp,CNRS, F-91191 Gif Sur Yvette, France
[2] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[3] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1090 GE Amsterdam, Netherlands
[4] Univ Sydney, Sch Phys, Sydney Inst Astron SIfA, Sydney, NSW 2006, Australia
[5] Inst Astrofis Andalucia CSIC, Granada 18008, Spain
[6] Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark
[7] Univ Paris 09, Inst Astrophys Spatiale, CNRS, UMR8617, F-91405 Orsay, France
[8] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[9] Univ Toulouse, Lab Astrophys Toulouse Tarbes, CNRS, F-31400 Toulouse, France
[10] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[11] Univ Vienna, Inst Astron, A-1180 Vienna, Austria
[12] NASA, Ames Res Ctr, SETI Inst, Moffett Field, CA 94035 USA
[13] NASA, Ames Res Ctr, Orbital Sci Corp, Moffett Field, CA 94035 USA
[14] Univ Wroclaw, Astron Inst, PL-51622 Wroclaw, Poland
[15] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal
基金
英国科学技术设施理事会;
关键词
asteroseismology; methods: data analysis; SOLAR-LIKE OSCILLATIONS; SUN-LIKE STAR; RED GIANTS; RADIUS DETERMINATION; COROT; MISSION; SCIENCE;
D O I
10.1111/j.1745-3933.2011.01042.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Kepler mission is providing photometric data of exquisite quality for the asteroseismic study of different classes of pulsating stars. These analyses place particular demands on the pre-processing of the data, over a range of time-scales from minutes to months. Here, we describe processing procedures developed by the Kepler Asteroseismic Science Consortium to prepare light curves that are optimized for the asteroseismic study of solar-like oscillating stars in which outliers, jumps and drifts are corrected.
引用
收藏
页码:L6 / L10
页数:5
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