TY - JOUR
T1 - TRANSIT TIMING OBSERVATIONS from KEPLER. IX. CATALOG of the FULL LONG-CADENCE DATA SET
AU - Holczer, Tomer
AU - Mazeh, Tsevi
AU - Nachmani, Gil
AU - Jontof-Hutter, Daniel
AU - Ford, Eric B.
AU - Fabrycky, Daniel
AU - Ragozzine, Darin
AU - Kane, Mackenzie
AU - Steffen, Jason H.
N1 - Funding Information:
The research leading to these results has received funding from the European Research Council under the EUs Seventh Framework Programme (FP7/(2007-2013)/ERC Grant Agreement No. 291352), the Israel SCIENCE FOUNDATION (grant No. 1423/11), and the Israeli Centers of Research Excellence (I-CORE, grant No. 1829/12).
Publisher Copyright:
© 2016. The American Astronomical Society. All rights reserved..
PY - 2016/7
Y1 - 2016/7
N2 - We present a new transit timing catalog of 2599 Kepler Objects of Interest (KOIs), using the PDC-MAP long-cadence light curves that include the full 17 quarters of the mission (ftp://wise-ftp.tau.ac.il/pub/tauttv/TTV/ver-112). The goal is to produce an easy-to-use catalog that can stimulate further analyses of interesting systems. For 779 KOIs with high enough S/N, we derived the timing, duration, and depth of 69,914 transits. For 1820 KOIs with lower SNR, we derived only the timing of 225,273 transits. After removal of outlier timings, we derived various statistics for each KOI that were used to indicate significant variations. Including systems found by previous works, we have detected 260 KOIs that showed significant TTVs with long-term variations (>100 days), and another 14 KOIs with periodic modulations shorter than 100 days and small amplitudes. For five of those, the periodicity is probably due to the crossing of rotating stellar spots by the transiting planets.
AB - We present a new transit timing catalog of 2599 Kepler Objects of Interest (KOIs), using the PDC-MAP long-cadence light curves that include the full 17 quarters of the mission (ftp://wise-ftp.tau.ac.il/pub/tauttv/TTV/ver-112). The goal is to produce an easy-to-use catalog that can stimulate further analyses of interesting systems. For 779 KOIs with high enough S/N, we derived the timing, duration, and depth of 69,914 transits. For 1820 KOIs with lower SNR, we derived only the timing of 225,273 transits. After removal of outlier timings, we derived various statistics for each KOI that were used to indicate significant variations. Including systems found by previous works, we have detected 260 KOIs that showed significant TTVs with long-term variations (>100 days), and another 14 KOIs with periodic modulations shorter than 100 days and small amplitudes. For five of those, the periodicity is probably due to the crossing of rotating stellar spots by the transiting planets.
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U2 - 10.3847/0067-0049/225/1/9
DO - 10.3847/0067-0049/225/1/9
M3 - Article
AN - SCOPUS:84980332137
SN - 0067-0049
VL - 225
JO - Astrophysical Journal, Supplement Series
JF - Astrophysical Journal, Supplement Series
IS - 1
M1 - 9
ER -