HAT-P-39bHAT-P-41b: Three highly inflated transiting hot Jupiters

J. D. Hartman; G. Á Bakos; B. Béky; G. Torres; D. W. Latham; Z. Csubry; K. Penev; A. Shporer; B. J. Fulton; L. A. Buchhave; J. A. Johnson; A. W. Howard; G. W. Marcy; D. A. Fischer; G. Kovács; R. W. Noyes; G. A. Esquerdo; M. Everett; T. Szklenár; S. N. Quinn; A. Bieryla; R. P. Knox; P. Hinz; D. D. Sasselov; G. Frész; R. P. Stefanik; J. Lázár; I. Papp; P. Sári

doi:10.1088/0004-6256/144/5/139

HAT-P-39bHAT-P-41b: Three highly inflated transiting hot Jupiters

J. D. Hartman
, G. Á Bakos
, B. Béky
, G. Torres
, D. W. Latham
, Z. Csubry
, K. Penev
, A. Shporer
, B. J. Fulton
, L. A. Buchhave
, J. A. Johnson
, A. W. Howard
, G. W. Marcy
, D. A. Fischer
, G. Kovács
, R. W. Noyes
, G. A. Esquerdo
, M. Everett
, T. Szklenár
, S. N. Quinn

A. Bieryla, R. P. Knox, P. Hinz, D. D. Sasselov, G. Frész, R. P. Stefanik, J. Lázár, I. Papp, P. Sári

Astrophysical Sciences

Research output: Contribution to journal › Article › peer-review

96 Scopus citations

Abstract

We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M _J,0.62M _J, and 0.80M _J, and radii of 1.57R _J,1.73R _J, and 1.68R _J, respectively. They orbit stars with masses of 1.40M _⊙,1.51M _⊙, and 1.51M _⊙, respectively. The three planets are members of an emerging population of highly inflated Jupiters with 0.4 M _J < M < 1.5 M _J and R > 1.5 R _J.

Original language	English (US)
Article number	139
Journal	Astronomical Journal
Volume	144
Issue number	5
DOIs	https://doi.org/10.1088/0004-6256/144/5/139
State	Published - Nov 2012

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

planetary systems
stars: individual (GSC 1364-01424, GSC 3607-01028, GSC 0488-02442)
techniques: photometric
techniques: spectroscopic

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Hartman, J. D., Bakos, G. Á., Béky, B., Torres, G., Latham, D. W., Csubry, Z., Penev, K., Shporer, A., Fulton, B. J., Buchhave, L. A., Johnson, J. A., Howard, A. W., Marcy, G. W., Fischer, D. A., Kovács, G., Noyes, R. W., Esquerdo, G. A., Everett, M., Szklenár, T., ... Sári, P. (2012). HAT-P-39bHAT-P-41b: Three highly inflated transiting hot Jupiters. Astronomical Journal, 144(5), Article 139. https://doi.org/10.1088/0004-6256/144/5/139

@article{72c20525b2064e468a3560d5f97c1764,

title = "HAT-P-39bHAT-P-41b: Three highly inflated transiting hot Jupiters",

abstract = "We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M J,0.62M J, and 0.80M J, and radii of 1.57R J,1.73R J, and 1.68R J, respectively. They orbit stars with masses of 1.40M ⊙,1.51M ⊙, and 1.51M ⊙, respectively. The three planets are members of an emerging population of highly inflated Jupiters with 0.4 M J < M < 1.5 M J and R > 1.5 R J.",

keywords = "planetary systems, stars: individual (GSC 1364-01424, GSC 3607-01028, GSC 0488-02442), techniques: photometric, techniques: spectroscopic",

author = "Hartman, \{J. D.\} and Bakos, \{G. {\'A}\} and B. B{\'e}ky and G. Torres and Latham, \{D. W.\} and Z. Csubry and K. Penev and A. Shporer and Fulton, \{B. J.\} and Buchhave, \{L. A.\} and Johnson, \{J. A.\} and Howard, \{A. W.\} and Marcy, \{G. W.\} and Fischer, \{D. A.\} and G. Kov{\'a}cs and Noyes, \{R. W.\} and Esquerdo, \{G. A.\} and M. Everett and T. Szklen{\'a}r and Quinn, \{S. N.\} and A. Bieryla and Knox, \{R. P.\} and P. Hinz and Sasselov, \{D. D.\} and G. Fr{\'e}sz and Stefanik, \{R. P.\} and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2012",

month = nov,

doi = "10.1088/0004-6256/144/5/139",

language = "English (US)",

volume = "144",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "5",

}

Hartman, JD , Bakos, GÁ, Béky, B, Torres, G, Latham, DW, Csubry, Z, Penev, K, Shporer, A, Fulton, BJ, Buchhave, LA, Johnson, JA, Howard, AW, Marcy, GW, Fischer, DA, Kovács, G, Noyes, RW, Esquerdo, GA, Everett, M, Szklenár, T, Quinn, SN, Bieryla, A, Knox, RP, Hinz, P, Sasselov, DD, Frész, G, Stefanik, RP, Lázár, J, Papp, I & Sári, P 2012, 'HAT-P-39bHAT-P-41b: Three highly inflated transiting hot Jupiters', Astronomical Journal, vol. 144, no. 5, 139. https://doi.org/10.1088/0004-6256/144/5/139

TY - JOUR

T1 - HAT-P-39bHAT-P-41b

T2 - Three highly inflated transiting hot Jupiters

AU - Hartman, J. D.

AU - Bakos, G. Á

AU - Béky, B.

AU - Torres, G.

AU - Latham, D. W.

AU - Csubry, Z.

AU - Penev, K.

AU - Shporer, A.

AU - Fulton, B. J.

AU - Buchhave, L. A.

AU - Johnson, J. A.

AU - Howard, A. W.

AU - Marcy, G. W.

AU - Fischer, D. A.

AU - Kovács, G.

AU - Noyes, R. W.

AU - Esquerdo, G. A.

AU - Everett, M.

AU - Szklenár, T.

AU - Quinn, S. N.

AU - Bieryla, A.

AU - Knox, R. P.

AU - Hinz, P.

AU - Sasselov, D. D.

AU - Frész, G.

AU - Stefanik, R. P.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2012/11

Y1 - 2012/11

N2 - We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M J,0.62M J, and 0.80M J, and radii of 1.57R J,1.73R J, and 1.68R J, respectively. They orbit stars with masses of 1.40M ⊙,1.51M ⊙, and 1.51M ⊙, respectively. The three planets are members of an emerging population of highly inflated Jupiters with 0.4 M J < M < 1.5 M J and R > 1.5 R J.

AB - We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M J,0.62M J, and 0.80M J, and radii of 1.57R J,1.73R J, and 1.68R J, respectively. They orbit stars with masses of 1.40M ⊙,1.51M ⊙, and 1.51M ⊙, respectively. The three planets are members of an emerging population of highly inflated Jupiters with 0.4 M J < M < 1.5 M J and R > 1.5 R J.

KW - planetary systems

KW - stars: individual (GSC 1364-01424, GSC 3607-01028, GSC 0488-02442)

KW - techniques: photometric

KW - techniques: spectroscopic

UR - https://www.scopus.com/pages/publications/84867323986

UR - https://www.scopus.com/pages/publications/84867323986#tab=citedBy

U2 - 10.1088/0004-6256/144/5/139

DO - 10.1088/0004-6256/144/5/139

M3 - Article

AN - SCOPUS:84867323986

SN - 0004-6256

VL - 144

JO - Astronomical Journal

JF - Astronomical Journal

IS - 5

M1 - 139

ER -

HAT-P-39bHAT-P-41b: Three highly inflated transiting hot Jupiters

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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