DETECTION OF POTENTIAL TRANSIT SIGNALS IN 16 QUARTERS OF KEPLER MISSION DATA

被引:31
|
作者
Tenenbaum, Peter [1 ]
Jenkins, Jonm. [1 ]
Seader, Shawn [1 ]
Burke, Christopher J. [1 ]
Christiansen, Jessie L. [1 ]
Rowe, Jason F. [1 ]
Caldwell, Douglas A. [1 ]
Clarke, Bruce D. [1 ]
Coughlin, Jeffrey L. [1 ]
Li, Jie [1 ]
Quintana, Elisa V. [1 ]
Smith, Jeffrey C. [1 ]
Thompson, Susan E. [1 ]
Twicken, Joseph D. [1 ]
Haas, Michael R. [2 ]
Henze, Christopher E. [2 ]
Hunter, Roger C. [2 ]
Sanderfer, Dwight T. [2 ]
Campbell, Jennifer R. [3 ]
Girouard, Forrest R. [3 ]
Klaus, Todd C. [3 ]
McCauliff, Sean D. [3 ]
Middour, Christopher K. [3 ]
Sabale, Anima [3 ]
Uddin, Akm Kamal [3 ]
Wohler, Bill [3 ]
Barclay, Thomas [4 ]
Still, Martin [4 ]
机构
[1] NASA, SETI Inst, Ames Res Ctr, Moffett Field, CA 94305 USA
[2] NASA, Ames Res Ctr, Moffett Field, CA 94305 USA
[3] NASA, Orbital Sci Corp, Ames Res Ctr, Moffett Field, CA 94305 USA
[4] NASA, BAER Inst, Ames Res Ctr, Moffett Field, CA 94305 USA
来源
关键词
planetary systems; planets and satellites: detection; SYSTEMATIC-ERROR CORRECTION; PLANETS;
D O I
10.1088/0067-0049/211/1/6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of a search for potential transit signals in 4 yr of photometry data acquired by the Kepler mission. The targets of the search include 111,800 stars which were observed for the entire interval and 85,522 stars which were observed for a subset of the interval. We found that 9743 targets contained at least one signal consistent with the signature of a transiting or eclipsing object where the criteria for detection are periodicity of the detected transits, adequate signal-to-noise ratio, and acceptance by a number of tests which reject false positive detections. When targets that had produced a signal were searched repeatedly, an additional 6542 signals were detected on 3223 target stars, for a total of 16,285 potential detections. Comparison of the set of detected signals with a set of known and vetted transit events in the Kepler field of view shows that the recovery rate for these signals is 96.9%. The ensemble properties of the detected signals are reviewed.
引用
收藏
页数:11
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