HAT-P-34b-HAT-P-37b: Four Transiting Planets More Massive than Jupiter Orbiting Moderately Bright Stars

• Published in: The Astronomical Journal
• Main Authors: Bakos, G. Ã., Hartman, J. D., Torres, G., Béky, B., Latham, D. W., Buchhave, L. A., Csubry, Z., Kovács, G., Bieryla, A., Quinn, S., Szklenár, T., Esquerdo, G. A., Shporer, A., Noyes, R. W., Fischer, D. A., Johnson, J. A., Howard, A. W., Marcy, G. W., Sato, B., Penev, K., Everett, M., Sasselov, D. D., Fűrész, G., Stefanik, R. P., Lázár, J., Papp, I., Sári, P.
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: American Astronomical Society 2012
• Subjects: planetary systems; stars: individual (HAT-P-34; GSC 1622-01261; HAT-P-35; GSC 0203-01079; HAT-P-36); techniques: photometric; techniques: spectroscopic; Norway; Jupiter; Observatorio; Iceland
• Online Access: https://doi.org/10.1088/0004-6256/144/1/19

We report the discovery of four transiting extrasolar planets (HAT-P-34b–HAT-P-37b) with masses ranging from 1.05 to 3.33 M_J and periods from 1.33 to 5.45 days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is mod...