{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2022,4,5]],"date-time":"2022-04-05T05:01:45Z","timestamp":1649134905275},"reference-count":4,"publisher":"Cambridge University Press (CUP)","issue":"S276","license":[{"start":{"date-parts":[[2011,11,10]],"date-time":"2011-11-10T00:00:00Z","timestamp":1320883200000},"content-version":"unspecified","delay-in-days":405,"URL":"https:\/\/www.cambridge.org\/core\/terms"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Proc. IAU"],"published-print":{"date-parts":[[2010,10]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>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 <jats:italic>Kepler<\/jats:italic> 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 <jats:italic>Kepler<\/jats:italic> space telescope. We have used four criteria, namely, the magnitude, proper motion, <jats:italic>H-K<\/jats:italic><jats:sub><jats:italic>s<\/jats:italic><\/jats:sub> and <jats:italic>J-H<\/jats:italic> 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 <jats:italic>Kepler<\/jats:italic>'s targets. We discuss the details of our selection process and present the results.<\/jats:p>","DOI":"10.1017\/s1743921311020746","type":"journal-article","created":{"date-parts":[[2011,11,10]],"date-time":"2011-11-10T04:32:19Z","timestamp":1320899539000},"page":"448-449","source":"Crossref","is-referenced-by-count":1,"title":["A survey of M stars in the field of view of <i>Kepler<\/i> space telescope"],"prefix":"10.1017","volume":"6","author":[{"given":"Mahmoudreza","family":"Oshagh","sequence":"first","affiliation":[]},{"given":"Nader","family":"Haghighipour","sequence":"additional","affiliation":[]},{"given":"Nuno C.","family":"Santos","sequence":"additional","affiliation":[]}],"member":"56","published-online":{"date-parts":[[2011,11,10]]},"reference":[{"key":"S1743921311020746_ref4","first-page":"475","volume":"398","author":"Traub","year":"2008","journal-title":"ASP Conf. Ser."},{"key":"S1743921311020746_ref1","doi-asserted-by":"publisher","DOI":"10.1088\/2041-8205\/713\/2\/L109"},{"key":"S1743921311020746_ref2","doi-asserted-by":"publisher","DOI":"10.1088\/0004-637X\/730\/2\/79"},{"key":"S1743921311020746_ref3","doi-asserted-by":"publisher","DOI":"10.1086\/191720"}],"container-title":["Proceedings of the International Astronomical Union"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.cambridge.org\/core\/services\/aop-cambridge-core\/content\/view\/S1743921311020746","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2019,4,27]],"date-time":"2019-04-27T17:31:21Z","timestamp":1556386281000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.cambridge.org\/core\/product\/identifier\/S1743921311020746\/type\/journal_article"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2010,10]]},"references-count":4,"journal-issue":{"issue":"S276","published-print":{"date-parts":[[2010,10]]}},"alternative-id":["S1743921311020746"],"URL":"https:\/\/doi.org\/10.1017\/s1743921311020746","relation":{},"ISSN":["1743-9213","1743-9221"],"issn-type":[{"value":"1743-9213","type":"print"},{"value":"1743-9221","type":"electronic"}],"subject":[],"published":{"date-parts":[[2010,10]]}}}