{ "id": "1012.2234", "version": "v1", "published": "2010-12-10T11:22:38.000Z", "updated": "2010-12-10T11:22:38.000Z", "title": "A Survey of M Stars in the Field of View of Kepler Space Telescope", "authors": [ "Mahmoudreza Oshagh", "Nader Haghighipour", "Nuno C. Santos" ], "comment": "2 pages, 1 table, To be published in proceedings of the IAU Symposium No.276", "journal": "The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomical Union, IAU Symposium, 276, 448-449 (2011)", "doi": "10.1017/S1743921311020746", "categories": [ "astro-ph.EP" ], "abstract": "M dwarfs constitute more than 70% of the stars in the solar neighborhood. They are cooler and smaller than Sun-like stars and have less-massive disks which suggests that planets around these stars are more likely to be Neptune-size or smaller. The transit depths and transit times of planets around M stars are large and well-matched to the Kepler temporal resolution. As a result, M stars have been of particular interest for searching for planets in both radial velocity and transit photometry surveys. We have recently started a project on searching for possible planet-hosting M stars in the publicly available data from Kepler space telescope. We have used four criteria, namely, the magnitude, proper motion, H-Ks and J-H colors, and searched for M stars in Q0 and Q1 data sets. We have been able to find 108 M stars among which 54 had not been previously identified among Kepler's targets. We discuss the details of our selection process and present the results.", "revisions": [ { "version": "v1", "updated": "2010-12-10T11:22:38.000Z" } ], "analyses": { "keywords": [ "kepler space telescope", "kepler temporal resolution", "transit photometry surveys", "q1 data sets", "transit times" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 2, "language": "en", "license": "arXiv", "status": "editable", "inspire": 880915, "adsabs": "2011IAUS..276..448O" } } }