Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-12-07
Astron.J.131:1090-1105,2006
Astronomy and Astrophysics
Astrophysics
21 pages LaTeX, including 14 figures and 7 tables. To be published in the February 2006 Astronomical Journal. Paper with bette
Scientific paper
10.1086/499208
We have undertaken a long-term project, Planets in Stellar Clusters Extensive Search (PISCES), to search for transiting planets in open clusters. In this paper we present the results for NGC 2158, an intermediate age, populous cluster. We have monitored the cluster for over 260 hours, spread over 59 nights. We have detected one candidate transiting low luminosity object, with eclipse depth of 3.7% in the R-band. If the host star is a member of the cluster, the eclipse depth is consistent with a 1.7 R_J object. Cluster membership of the host is supported by its location on the cluster main sequence (MS) and its close proximity to the cluster center (2'). We have discovered two other stars exhibiting low-amplitude (4-5%) transits, V64 and V70, but they are most likely blends or field stars. Given the photometric precision and temporal coverage of our observations, and current best estimates for the frequency and radii of short-period planets, the expected number of detectable transiting planets in our sample is 0.13. We have observed four outbursts for the candidate cataclysmic variable V57. We have discovered 40 new variable stars in the cluster, bringing the total number of identified variables to 97, and present for them high precision light curves, spanning 13 months.
Adams Elisabeth
Cooper Randall L.
Foster Jonathan B.
Hartman Joel D.
Hickox Ryan C.
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