HATS-13b and HATS-14b: Two transiting hot Jupiters from the HATSouth survey

L. Mancini; J. D. Hartman; K. Penev; G. A. Bakos; R. Brahm; S. Ciceri; T. Henning; Z. Csubry; D. Bayliss; G. Zhou; M. Rabus; M. De Val-Borro; N. Espinoza; A. Jordan; V. Suc; W. Bhatti; B. Schmidt; B. Sato; T. G. Tan; D. J. Wright; C. G. Tinney; B. C. Addison; R. W. Noyes; J. Lazar; I. Papp; P. Sari

doi:10.1051/0004-6361/201526069

HATS-13b and HATS-14b: Two transiting hot Jupiters from the HATSouth survey

L. Mancini
, J. D. Hartman
, K. Penev
, G. A. Bakos
, R. Brahm
, S. Ciceri
, T. Henning
, Z. Csubry
, D. Bayliss
, G. Zhou
, M. Rabus
, M. De Val-Borro
, N. Espinoza
, A. Jordan
, V. Suc
, W. Bhatti
, B. Schmidt
, B. Sato
, T. G. Tan
, D. J. Wright

C. G. Tinney, B. C. Addison, R. W. Noyes, J. Lazar, I. Papp, P. Sari

Research output: Contribution to journal › Review article › peer-review

18 Scopus citations

Abstract

We report the discovery of HATS-13b and HATS-14b, which are 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_z.ast; = 0.96 M_⊙, R_z.ast; = 0.89 R_⊙, T_eff ≈ 5500 K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, M_z.ast; = 0.97 M_⊙, R_z.ast; = 0.93 R_⊙, T_eff ≈ 5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of ~3 days and a separation of ~0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. HATS-13b, with a mass of M_p = 0.543 ± 0.072 M_J and a radius of R_p = 1.212 ± 0.035 R_J, appears as an inflated planet, while HATS-14b, having a mass of M_p = 1.071 ± 0.070 M_J and a radius of R_p = 1.039 ± 0.032 R_J, is only slightly larger in radius than Jupiter.

Original language	English
Article number	A63
Journal	Astronomy and Astrophysics
Volume	580
DOIs	https://doi.org/10.1051/0004-6361/201526069
State	Published - 1 Aug 2015
Externally published	Yes

Keywords

Planetary systems
Stars: fundamental parameters
Stars: individual: HATS-13 (aka GSC6928-00497)
Stars: individual: HATS-14 (aka GSC6926-00259)
Techniques: photometric
Techniques: radial velocities

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Mancini, L., Hartman, J. D., Penev, K., Bakos, G. A., Brahm, R., Ciceri, S., Henning, T., Csubry, Z., Bayliss, D., Zhou, G., Rabus, M., De Val-Borro, M., Espinoza, N., Jordan, A., Suc, V., Bhatti, W., Schmidt, B., Sato, B., Tan, T. G., ... Sari, P. (2015). HATS-13b and HATS-14b: Two transiting hot Jupiters from the HATSouth survey. Astronomy and Astrophysics, 580, Article A63. https://doi.org/10.1051/0004-6361/201526069

@article{501b021a9c17464e8d911a641b65ab21,

title = "HATS-13b and HATS-14b: Two transiting hot Jupiters from the HATSouth survey",

abstract = "We report the discovery of HATS-13b and HATS-14b, which are 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, Mz.ast; = 0.96 M⊙, Rz.ast; = 0.89 R⊙, Teff ≈ 5500 K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, Mz.ast; = 0.97 M⊙, Rz.ast; = 0.93 R⊙, Teff ≈ 5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of \textasciitilde{}3 days and a separation of \textasciitilde{}0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. HATS-13b, with a mass of Mp = 0.543 ± 0.072 MJ and a radius of Rp = 1.212 ± 0.035 RJ, appears as an inflated planet, while HATS-14b, having a mass of Mp = 1.071 ± 0.070 MJ and a radius of Rp = 1.039 ± 0.032 RJ, is only slightly larger in radius than Jupiter.",

keywords = "Planetary systems, Stars: fundamental parameters, Stars: individual: HATS-13 (aka GSC6928-00497), Stars: individual: HATS-14 (aka GSC6926-00259), Techniques: photometric, Techniques: radial velocities",

author = "L. Mancini and Hartman, \{J. D.\} and K. Penev and Bakos, \{G. A.\} and R. Brahm and S. Ciceri and T. Henning and Z. Csubry and D. Bayliss and G. Zhou and M. Rabus and \{De Val-Borro\}, M. and N. Espinoza and A. Jordan and V. Suc and W. Bhatti and B. Schmidt and B. Sato and Tan, \{T. G.\} and Wright, \{D. J.\} and Tinney, \{C. G.\} and Addison, \{B. C.\} and Noyes, \{R. W.\} and J. Lazar and I. Papp and P. Sari",

note = "Publisher Copyright: {\textcopyright} 2015 ESO.",

year = "2015",

month = aug,

day = "1",

doi = "10.1051/0004-6361/201526069",

language = "English",

volume = "580",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Mancini, L, Hartman, JD, Penev, K, Bakos, GA, Brahm, R, Ciceri, S, Henning, T, Csubry, Z, Bayliss, D, Zhou, G, Rabus, M, De Val-Borro, M, Espinoza, N, Jordan, A, Suc, V, Bhatti, W, Schmidt, B, Sato, B, Tan, TG, Wright, DJ, Tinney, CG, Addison, BC, Noyes, RW, Lazar, J, Papp, I & Sari, P 2015, 'HATS-13b and HATS-14b: Two transiting hot Jupiters from the HATSouth survey', Astronomy and Astrophysics, vol. 580, A63. https://doi.org/10.1051/0004-6361/201526069

TY - JOUR

T1 - HATS-13b and HATS-14b

T2 - Two transiting hot Jupiters from the HATSouth survey

AU - Mancini, L.

AU - Hartman, J. D.

AU - Penev, K.

AU - Bakos, G. A.

AU - Brahm, R.

AU - Ciceri, S.

AU - Henning, T.

AU - Csubry, Z.

AU - Bayliss, D.

AU - Zhou, G.

AU - Rabus, M.

AU - De Val-Borro, M.

AU - Espinoza, N.

AU - Jordan, A.

AU - Suc, V.

AU - Bhatti, W.

AU - Schmidt, B.

AU - Sato, B.

AU - Tan, T. G.

AU - Wright, D. J.

AU - Tinney, C. G.

AU - Addison, B. C.

AU - Noyes, R. W.

AU - Lazar, J.

AU - Papp, I.

AU - Sari, P.

PY - 2015/8/1

Y1 - 2015/8/1

N2 - We report the discovery of HATS-13b and HATS-14b, which are 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, Mz.ast; = 0.96 M⊙, Rz.ast; = 0.89 R⊙, Teff ≈ 5500 K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, Mz.ast; = 0.97 M⊙, Rz.ast; = 0.93 R⊙, Teff ≈ 5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of ~3 days and a separation of ~0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. HATS-13b, with a mass of Mp = 0.543 ± 0.072 MJ and a radius of Rp = 1.212 ± 0.035 RJ, appears as an inflated planet, while HATS-14b, having a mass of Mp = 1.071 ± 0.070 MJ and a radius of Rp = 1.039 ± 0.032 RJ, is only slightly larger in radius than Jupiter.

AB - We report the discovery of HATS-13b and HATS-14b, which are 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, Mz.ast; = 0.96 M⊙, Rz.ast; = 0.89 R⊙, Teff ≈ 5500 K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, Mz.ast; = 0.97 M⊙, Rz.ast; = 0.93 R⊙, Teff ≈ 5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of ~3 days and a separation of ~0.04 au. However, even though they are irradiated in a similar way, the physical characteristics of the two planets are very different. HATS-13b, with a mass of Mp = 0.543 ± 0.072 MJ and a radius of Rp = 1.212 ± 0.035 RJ, appears as an inflated planet, while HATS-14b, having a mass of Mp = 1.071 ± 0.070 MJ and a radius of Rp = 1.039 ± 0.032 RJ, is only slightly larger in radius than Jupiter.

KW - Planetary systems

KW - Stars: fundamental parameters

KW - Stars: individual: HATS-13 (aka GSC6928-00497)

KW - Stars: individual: HATS-14 (aka GSC6926-00259)

KW - Techniques: photometric

KW - Techniques: radial velocities

UR - https://www.scopus.com/pages/publications/84938585172

U2 - 10.1051/0004-6361/201526069

DO - 10.1051/0004-6361/201526069

M3 - Review article

AN - SCOPUS:84938585172

SN - 0004-6361

VL - 580

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A63

ER -

HATS-13b and HATS-14b: Two transiting hot Jupiters from the HATSouth survey

Abstract

Keywords

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