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Hartman, J.F. Kielkopf, J. L\\'az\\'ar, J.M. Jenkins, J.N. Winn, K.A. Collins, K. Barkaoui, K.G. Stassun, K. Haworth, K. Horne, K.I. Collins, K. Penev, Lars A. Buchhave, L.D. Nielsen, M.C. Johnson, M. Davies, M. de Val-Borro, M. Everett, M. Gillon, M.L. Calkins, N. Espinoza, N. Guerrero, N. Narita, N. Schanche, P. Berlind, P. S\\'ari, R.G. West, R. Hart, Robert F. Goeke, R. Sefako, R. Vanderspek, R.W. Noyes, S.B. Howell, S.N. Quinn, S. Seager, S. Villanueva, T. Gan, T.G. Tan, T. Kov\\'acs, T. Nishiumi, T. Szklen\\'ar, W. Bhatti, W.D. Cochran, Z. Benkhaldoun, Z. Csubry","submitted_at":"2019-06-02T18:00:02Z","abstract_excerpt":"Wide field surveys for transiting planets are well suited to searching diverse stellar populations, enabling a better understanding of the link between the properties of planets and their parent stars. 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