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
State	Published - Feb 2019
Externally published	Yes

Keywords

stars: individual
techniques: photometric
techniques: spectroscopic

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10.3847/1538-3881/aaf8b6

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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

@article{0bd0961384ac4faf804fc6906a68b11e,

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",

note = "Funding Information: We thank the anonymous referee for their careful review of our paper, which has significantly improved its quality. Development of the HATSouth project was funded by NSF MRI grant NSF/AST-0723074; operations have been supported by NASA grants NNX09AB29G, NNX12AH91H, and NNX17AB61G; and follow-up observations have received partial support from grant NSF/AST-1108686. A.J. acknowledges support from FONDECYT project 1171208, BASAL CATA PFB-06, and project IC120009 “Millennium Institute of Astrophysics (MAS)” of the Millennium Science Initiative, Chilean Ministry of Economy. N.E. is supported by CON-ICYT-PCHA/Doctorado Nacional. R.B. acknowledges support from FONDECYT Post-doctoral Fellowship Project no. 3180246. N.E. acknowledges support from project IC120009 “Millennium Institute of Astrophysics (MAS)” of the Millennium Science Initiative, Chilean Ministry of Economy. L.M. acknowledges support from the Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund. L.M. acknowledges support from the University of Rome Tor Vergata through the “Mission: Sustainability 2016” fund. V.S. acknowledges support from BASAL CATA PFB-06. A.V. is supported by the NSF Graduate Research Fellowship, grant no. DGE 1144152. This work is based on observations made with ESO Telescopes at the La Silla Observatory. This paper also makes use of observations from the LCOGT network. Some of this time was awarded by NOAO. We acknowledge the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund, and the SIMBAD database, operated at CDS, Strasbourg, France. Operations at the MPG2.2 m Telescope are jointly performed by the Max Planck Gesellschaft and the European Southern Observatory. We thank the MPG 2.2 m telescope support team for their technical assistance during observations. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC,https:// www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Publisher Copyright: {\textcopyright} 2019. The American Astronomical Society. All rights reserved.",

year = "2019",

month = feb,

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

language = "English",

volume = "157",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "2",

}

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.

N1 - Funding Information: We thank the anonymous referee for their careful review of our paper, which has significantly improved its quality. Development of the HATSouth project was funded by NSF MRI grant NSF/AST-0723074; operations have been supported by NASA grants NNX09AB29G, NNX12AH91H, and NNX17AB61G; and follow-up observations have received partial support from grant NSF/AST-1108686. A.J. acknowledges support from FONDECYT project 1171208, BASAL CATA PFB-06, and project IC120009 “Millennium Institute of Astrophysics (MAS)” of the Millennium Science Initiative, Chilean Ministry of Economy. N.E. is supported by CON-ICYT-PCHA/Doctorado Nacional. R.B. acknowledges support from FONDECYT Post-doctoral Fellowship Project no. 3180246. N.E. acknowledges support from project IC120009 “Millennium Institute of Astrophysics (MAS)” of the Millennium Science Initiative, Chilean Ministry of Economy. L.M. acknowledges support from the Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund. L.M. acknowledges support from the University of Rome Tor Vergata through the “Mission: Sustainability 2016” fund. V.S. acknowledges support from BASAL CATA PFB-06. A.V. is supported by the NSF Graduate Research Fellowship, grant no. DGE 1144152. This work is based on observations made with ESO Telescopes at the La Silla Observatory. This paper also makes use of observations from the LCOGT network. Some of this time was awarded by NOAO. We acknowledge the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund, and the SIMBAD database, operated at CDS, Strasbourg, France. Operations at the MPG2.2 m Telescope are jointly performed by the Max Planck Gesellschaft and the European Southern Observatory. We thank the MPG 2.2 m telescope support team for their technical assistance during observations. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC,https:// www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Publisher Copyright: © 2019. The American Astronomical Society. All rights reserved.

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

AN - SCOPUS:85062913179

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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