HAT-P-42b and HAT-P-43b: two inflated transiting hot Jupiters from the HATNet survey

I. Boisse; J. D. Hartman; G. Á. Bakos; K. Penev; Z. Csubry; B. Béky; D. W. Latham; A. Bieryla; G. Torres; G. Kovács; Lars A. Buchhave; Terese Hansen; M. Everett; G. A. Esquerdo; T. Szklenár; E. Falco; A. Shporer; B. J. Fulton; R. W. Noyes; R. P. Stefanik; J. Lázár; I. Papp; P. Sári

doi:10.1051/0004-6361/201220993

HAT-P-42b and HAT-P-43b: two inflated transiting hot Jupiters from the HATNet survey

I. Boisse, J. D. Hartman, G. Á. Bakos, K. Penev, Z. Csubry, B. Béky, D. W. Latham, A. Bieryla, G. Torres, G. Kovács, Lars A. Buchhave, Terese Hansen, M. Everett, G. A. Esquerdo, T. Szklenár, E. Falco, A. Shporer, B. J. Fulton, R. W. Noyes, R. P. StefanikJ. Lázár, I. Papp, P. Sári

Astrophysics and Planetary Science

11 Citations (Scopus)

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Abstract

Aims. We announce the discovery of two new transiting planets, and provide their accurate initial characterization. Methods. First identified from the HATNet wide-field photometric survey, these candidate transiting planets were then followed-up with a variety of photometric observations. Determining the planetary nature of the objects and characterizing the parameters of the systems were mainly done with the SOPHIE spectrograph at the 1.93 m telescope at OHP and the TRES spectrograph at the 1.5 m telescope at FLWO. Results. HAT-P-42b and HAT-P-43b are typical hot Jupiters on circular orbits around early-G/late-F main sequence host stars, with periods of 4.641878 ± 0.000032 and 3.332687 ± 0.000015 days, masses of 0.044 ± 0.083 and 0.662 ± 0.060 M_J, and radii of 1.280 ± 0.153 and 1.281 _-0.033^{+ 0.062} R_J, respectively. These discoveries increase the sample of planets with measured mean densities, which are needed to constrain theories of planetary interiors and atmospheres. Moreover, their hosts are relatively bright (V < 13.5), which facilitates further follow-up studies.

Original language	English
Article number	A86
Journal	Astronomy & Astrophysics
Volume	558
Number of pages	10
ISSN	0004-6361
DOIs	https://doi.org/10.1051/0004-6361/201220993
Publication status	Published - 1 Oct 2013

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Boisse, I., Hartman, J. D., Bakos, G. Á., Penev, K., Csubry, Z., Béky, B., Latham, D. W., Bieryla, A., Torres, G., Kovács, G., Buchhave, L. A., Hansen, T., Everett, M., Esquerdo, G. A., Szklenár, T., Falco, E., Shporer, A., Fulton, B. J., Noyes, R. W., ... Sári, P. (2013). HAT-P-42b and HAT-P-43b: two inflated transiting hot Jupiters from the HATNet survey. Astronomy & Astrophysics, 558, Article A86. https://doi.org/10.1051/0004-6361/201220993

Boisse, I, Hartman, JD, Bakos, GÁ, Penev, K, Csubry, Z, Béky, B, Latham, DW, Bieryla, A, Torres, G, Kovács, G, Buchhave, LA , Hansen, T, Everett, M, Esquerdo, GA, Szklenár, T, Falco, E, Shporer, A, Fulton, BJ, Noyes, RW, Stefanik, RP, Lázár, J, Papp, I & Sári, P 2013, 'HAT-P-42b and HAT-P-43b: two inflated transiting hot Jupiters from the HATNet survey', Astronomy & Astrophysics, vol. 558, A86. https://doi.org/10.1051/0004-6361/201220993

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title = "HAT-P-42b and HAT-P-43b: two inflated transiting hot Jupiters from the HATNet survey",

abstract = "Aims. We announce the discovery of two new transiting planets, and provide their accurate initial characterization. Methods. First identified from the HATNet wide-field photometric survey, these candidate transiting planets were then followed-up with a variety of photometric observations. Determining the planetary nature of the objects and characterizing the parameters of the systems were mainly done with the SOPHIE spectrograph at the 1.93 m telescope at OHP and the TRES spectrograph at the 1.5 m telescope at FLWO. Results. HAT-P-42b and HAT-P-43b are typical hot Jupiters on circular orbits around early-G/late-F main sequence host stars, with periods of 4.641878 ± 0.000032 and 3.332687 ± 0.000015 days, masses of 0.044 ± 0.083 and 0.662 ± 0.060 MJ, and radii of 1.280 ± 0.153 and 1.281 -0.033+ 0.062 RJ, respectively. These discoveries increase the sample of planets with measured mean densities, which are needed to constrain theories of planetary interiors and atmospheres. Moreover, their hosts are relatively bright (V < 13.5), which facilitates further follow-up studies.",

author = "I. Boisse and Hartman, {J. D.} and Bakos, {G. {\'A}.} and K. Penev and Z. Csubry and B. B{\'e}ky and Latham, {D. W.} and A. Bieryla and G. Torres and G. Kov{\'a}cs and Buchhave, {Lars A.} and Terese Hansen and M. Everett and Esquerdo, {G. A.} and T. Szklen{\'a}r and E. Falco and A. Shporer and Fulton, {B. J.} and Noyes, {R. W.} and Stefanik, {R. P.} and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2013",

month = oct,

day = "1",

doi = "10.1051/0004-6361/201220993",

language = "English",

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TY - JOUR

T1 - HAT-P-42b and HAT-P-43b

T2 - two inflated transiting hot Jupiters from the HATNet survey

AU - Boisse, I.

AU - Hartman, J. D.

AU - Bakos, G. Á.

AU - Penev, K.

AU - Csubry, Z.

AU - Béky, B.

AU - Latham, D. W.

AU - Bieryla, A.

AU - Torres, G.

AU - Kovács, G.

AU - Buchhave, Lars A.

AU - Hansen, Terese

AU - Everett, M.

AU - Esquerdo, G. A.

AU - Szklenár, T.

AU - Falco, E.

AU - Shporer, A.

AU - Fulton, B. J.

AU - Noyes, R. W.

AU - Stefanik, R. P.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2013/10/1

Y1 - 2013/10/1

N2 - Aims. We announce the discovery of two new transiting planets, and provide their accurate initial characterization. Methods. First identified from the HATNet wide-field photometric survey, these candidate transiting planets were then followed-up with a variety of photometric observations. Determining the planetary nature of the objects and characterizing the parameters of the systems were mainly done with the SOPHIE spectrograph at the 1.93 m telescope at OHP and the TRES spectrograph at the 1.5 m telescope at FLWO. Results. HAT-P-42b and HAT-P-43b are typical hot Jupiters on circular orbits around early-G/late-F main sequence host stars, with periods of 4.641878 ± 0.000032 and 3.332687 ± 0.000015 days, masses of 0.044 ± 0.083 and 0.662 ± 0.060 MJ, and radii of 1.280 ± 0.153 and 1.281 -0.033+ 0.062 RJ, respectively. These discoveries increase the sample of planets with measured mean densities, which are needed to constrain theories of planetary interiors and atmospheres. Moreover, their hosts are relatively bright (V < 13.5), which facilitates further follow-up studies.

AB - Aims. We announce the discovery of two new transiting planets, and provide their accurate initial characterization. Methods. First identified from the HATNet wide-field photometric survey, these candidate transiting planets were then followed-up with a variety of photometric observations. Determining the planetary nature of the objects and characterizing the parameters of the systems were mainly done with the SOPHIE spectrograph at the 1.93 m telescope at OHP and the TRES spectrograph at the 1.5 m telescope at FLWO. Results. HAT-P-42b and HAT-P-43b are typical hot Jupiters on circular orbits around early-G/late-F main sequence host stars, with periods of 4.641878 ± 0.000032 and 3.332687 ± 0.000015 days, masses of 0.044 ± 0.083 and 0.662 ± 0.060 MJ, and radii of 1.280 ± 0.153 and 1.281 -0.033+ 0.062 RJ, respectively. These discoveries increase the sample of planets with measured mean densities, which are needed to constrain theories of planetary interiors and atmospheres. Moreover, their hosts are relatively bright (V < 13.5), which facilitates further follow-up studies.

U2 - 10.1051/0004-6361/201220993

DO - 10.1051/0004-6361/201220993

M3 - Journal article

SN - 0004-6361

VL - 558

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A86

ER -

HAT-P-42b and HAT-P-43b: two inflated transiting hot Jupiters from the HATNet survey

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