HATS-60b-HATS-69b: 10 Transiting Planets from HATSouth

J. D. Hartman; G. A. Bakos; D. Bayliss; J. Bento; W. Bhatti; R. Brahm; Z. Csubry; N. Espinoza; Th Henning; A. Jordán; L. Mancini; K. Penev; M. Rabus; P. Sarkis; V. Suc; M. De Val-Borro; G. Zhou; B. Addison; P. Arriagada; R. P. Butler; J. Crane; S. Durkan; S. Shectman; T. G. Tan; I. Thompson; C. G. Tinney; D. J. Wright; J. Lázár; I. Papp; P. Sári

doi:10.3847/1538-3881/aaf8b6

HATS-60b-HATS-69b: 10 Transiting Planets from HATSouth

J. D. Hartman, G. A. Bakos, D. Bayliss, J. Bento, W. Bhatti, R. Brahm, Z. Csubry, N. Espinoza, Th Henning, A. Jordán, L. Mancini, K. Penev, M. Rabus, P. Sarkis, V. Suc, M. De Val-Borro, G. Zhou, B. Addison, P. Arriagada, R. P. ButlerJ. Crane, S. Durkan, S. Shectman, T. G. Tan, I. Thompson, C. G. Tinney, D. J. Wright, J. Lázár, I. Papp, P. Sári

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Abstract

We report the discovery of 10 transiting extrasolar planets by the HATSouth survey. The planets range in mass from the super-Neptune HATS-62b, with M _p < 0.179 MJ, to the super-Jupiter HATS-66b, with M _p = 5.33M _J , and in size from the Saturn HATS-69b, with R _p = 0.94 R _J , to the inflated Jupiter HATS-67b, with R _p = 1.69 R _J . The planets have orbital periods between 1.6092 days (HATS-67b) and 7.8180 days (HATS-61b). The hosts are dwarf stars with masses ranging from 0.89 M _⊙ (HATS-69) to1.56 M _⊙ (HATS-64) and have apparent magnitudes between V = 12.276 ± 0.020 mag (HATS-68) and V = 14.095 ± 0.030 mag (HATS-66). The super-Neptune HATS-62b is the least massive planet discovered to date with a radius larger than Jupiter. Based largely on the Gaia DR2 distances and broadband photometry, we identify three systems (HATS-62, HATS-64, and HATS-65) as having possible unresolved binary star companions. We discuss in detail our methods for incorporating the Gaia DR2 observations into our modeling of the system parameters and into our blend analysis procedures.

Original language	English
Article number	55
Journal	Astronomical Journal
Volume	157
Issue number	2
DOIs	https://doi.org/10.3847/1538-3881/aaf8b6
Publication status	Published - Feb 2019

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Hartman, J. D., Bakos, G. A., Bayliss, D., Bento, J., Bhatti, W., Brahm, R., Csubry, Z., Espinoza, N., Henning, T., Jordán, A., Mancini, L., Penev, K., Rabus, M., Sarkis, P., Suc, V., Val-Borro, M. D., Zhou, G., Addison, B., Arriagada, P., ... Sári, P. (2019). HATS-60b-HATS-69b: 10 Transiting Planets from HATSouth. Astronomical Journal, 157(2), Article 55. https://doi.org/10.3847/1538-3881/aaf8b6

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title = "HATS-60b-HATS-69b: 10 Transiting Planets from HATSouth",

abstract = " We report the discovery of 10 transiting extrasolar planets by the HATSouth survey. The planets range in mass from the super-Neptune HATS-62b, with M p < 0.179 MJ, to the super-Jupiter HATS-66b, with M p = 5.33M J , and in size from the Saturn HATS-69b, with R p = 0.94 R J , to the inflated Jupiter HATS-67b, with R p = 1.69 R J . The planets have orbital periods between 1.6092 days (HATS-67b) and 7.8180 days (HATS-61b). The hosts are dwarf stars with masses ranging from 0.89 M ⊙ (HATS-69) to1.56 M ⊙ (HATS-64) and have apparent magnitudes between V = 12.276 ± 0.020 mag (HATS-68) and V = 14.095 ± 0.030 mag (HATS-66). The super-Neptune HATS-62b is the least massive planet discovered to date with a radius larger than Jupiter. Based largely on the Gaia DR2 distances and broadband photometry, we identify three systems (HATS-62, HATS-64, and HATS-65) as having possible unresolved binary star companions. We discuss in detail our methods for incorporating the Gaia DR2 observations into our modeling of the system parameters and into our blend analysis procedures.",

keywords = "stars: individual, techniques: photometric, techniques: spectroscopic",

author = "Hartman, {J. D.} and Bakos, {G. A.} and D. Bayliss and J. Bento and W. Bhatti and R. Brahm and Z. Csubry and N. Espinoza and Th Henning and A. Jord{\'a}n and L. Mancini and K. Penev and M. Rabus and P. Sarkis and V. Suc and Val-Borro, {M. De} and G. Zhou and B. Addison and P. Arriagada and Butler, {R. P.} and J. Crane and S. Durkan and S. Shectman and Tan, {T. G.} and I. Thompson and Tinney, {C. G.} and Wright, {D. J.} and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2019",

month = feb,

doi = "10.3847/1538-3881/aaf8b6",

language = "English",

volume = "157",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

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Hartman, JD, Bakos, GA, Bayliss, D, Bento, J, Bhatti, W, Brahm, R, Csubry, Z, Espinoza, N, Henning, T, Jordán, A, Mancini, L, Penev, K, Rabus, M, Sarkis, P, Suc, V, Val-Borro, MD, Zhou, G, Addison, B, Arriagada, P, Butler, RP, Crane, J, Durkan, S, Shectman, S, Tan, TG, Thompson, I, Tinney, CG, Wright, DJ, Lázár, J, Papp, I & Sári, P 2019, 'HATS-60b-HATS-69b: 10 Transiting Planets from HATSouth', Astronomical Journal, vol. 157, no. 2, 55. https://doi.org/10.3847/1538-3881/aaf8b6

TY - JOUR

T1 - HATS-60b-HATS-69b

T2 - 10 Transiting Planets from HATSouth

AU - Hartman, J. D.

AU - Bakos, G. A.

AU - Bayliss, D.

AU - Bento, J.

AU - Bhatti, W.

AU - Brahm, R.

AU - Csubry, Z.

AU - Espinoza, N.

AU - Henning, Th

AU - Jordán, A.

AU - Mancini, L.

AU - Penev, K.

AU - Rabus, M.

AU - Sarkis, P.

AU - Suc, V.

AU - Val-Borro, M. De

AU - Zhou, G.

AU - Addison, B.

AU - Arriagada, P.

AU - Butler, R. P.

AU - Crane, J.

AU - Durkan, S.

AU - Shectman, S.

AU - Tan, T. G.

AU - Thompson, I.

AU - Tinney, C. G.

AU - Wright, D. J.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2019/2

Y1 - 2019/2

N2 - We report the discovery of 10 transiting extrasolar planets by the HATSouth survey. The planets range in mass from the super-Neptune HATS-62b, with M p < 0.179 MJ, to the super-Jupiter HATS-66b, with M p = 5.33M J , and in size from the Saturn HATS-69b, with R p = 0.94 R J , to the inflated Jupiter HATS-67b, with R p = 1.69 R J . The planets have orbital periods between 1.6092 days (HATS-67b) and 7.8180 days (HATS-61b). The hosts are dwarf stars with masses ranging from 0.89 M ⊙ (HATS-69) to1.56 M ⊙ (HATS-64) and have apparent magnitudes between V = 12.276 ± 0.020 mag (HATS-68) and V = 14.095 ± 0.030 mag (HATS-66). The super-Neptune HATS-62b is the least massive planet discovered to date with a radius larger than Jupiter. Based largely on the Gaia DR2 distances and broadband photometry, we identify three systems (HATS-62, HATS-64, and HATS-65) as having possible unresolved binary star companions. We discuss in detail our methods for incorporating the Gaia DR2 observations into our modeling of the system parameters and into our blend analysis procedures.

AB - We report the discovery of 10 transiting extrasolar planets by the HATSouth survey. The planets range in mass from the super-Neptune HATS-62b, with M p < 0.179 MJ, to the super-Jupiter HATS-66b, with M p = 5.33M J , and in size from the Saturn HATS-69b, with R p = 0.94 R J , to the inflated Jupiter HATS-67b, with R p = 1.69 R J . The planets have orbital periods between 1.6092 days (HATS-67b) and 7.8180 days (HATS-61b). The hosts are dwarf stars with masses ranging from 0.89 M ⊙ (HATS-69) to1.56 M ⊙ (HATS-64) and have apparent magnitudes between V = 12.276 ± 0.020 mag (HATS-68) and V = 14.095 ± 0.030 mag (HATS-66). The super-Neptune HATS-62b is the least massive planet discovered to date with a radius larger than Jupiter. Based largely on the Gaia DR2 distances and broadband photometry, we identify three systems (HATS-62, HATS-64, and HATS-65) as having possible unresolved binary star companions. We discuss in detail our methods for incorporating the Gaia DR2 observations into our modeling of the system parameters and into our blend analysis procedures.

KW - stars: individual

KW - techniques: photometric

KW - techniques: spectroscopic

UR - http://www.scopus.com/inward/record.url?scp=85062913179&partnerID=8YFLogxK

U2 - 10.3847/1538-3881/aaf8b6

DO - 10.3847/1538-3881/aaf8b6

M3 - Article

SN - 0004-6256

VL - 157

JO - Astronomical Journal

JF - Astronomical Journal

IS - 2

M1 - 55

ER -

HATS-60b-HATS-69b: 10 Transiting Planets from HATSouth

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