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Csubry","submitted_at":"2015-03-11T19:58:15Z","abstract_excerpt":"We report the discovery of HATS-13b and HATS-14b, two hot-Jupiter transiting planets discovered by the HATSouth survey. The host stars are quite similar to each other (HATS-13: V = 13.9 mag, M* = 0.96 Msun, R* = 0.89 Rsun, Teff = 5500 K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, M* = 0.97 Msun, R* = 0.93 Rsun, Teff = 5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of roughly 3 days and a separation of roughly 0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. 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Jordan, B. C. Addison, B. Sato, B. Schmidt, C. G. Tinney, D. Bayliss, D. J. Wright, G. A. Bakos, G. Zhou, I. Papp, J. D. Hartman, J. Lazar, K. Penev, L. Mancini, M. de Val-Borro, M. Rabus, N. Espinoza, P. Sari, R. Brahm, R. W. Noyes, S. Ciceri, T. G. Tan, Th. Henning, V. Suc, W. Bhatti, Z. Csubry","submitted_at":"2015-03-11T19:58:15Z","abstract_excerpt":"We report the discovery of HATS-13b and HATS-14b, two hot-Jupiter transiting planets discovered by the HATSouth survey. The host stars are quite similar to each other (HATS-13: V = 13.9 mag, M* = 0.96 Msun, R* = 0.89 Rsun, Teff = 5500 K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, M* = 0.97 Msun, R* = 0.93 Rsun, Teff = 5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of roughly 3 days and a separation of roughly 0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. 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