HAT-P-34b-HAT-P-37b: Four transiting planets more massive than Jupiter orbiting moderately bright stars

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

doi:10.1088/0004-6256/144/1/19

HAT-P-34b-HAT-P-37b: Four transiting planets more massive than Jupiter orbiting moderately bright stars

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

Astrophysical Sciences

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Abstract

We report the discovery of four transiting extrasolar planets (HAT-P-34b-HAT-P-37b) with masses ranging from 1.05 to 3.33M _J and periods from 1.33 to 5.45days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33M _J), has a high eccentricity of e = 0.441 ± 0.032 at a period of P = 5.452654 ± 0.000016 days, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.

Original language	English (US)
Article number	19
Journal	Astronomical Journal
Volume	144
Issue number	1
DOIs	https://doi.org/10.1088/0004-6256/144/1/19
State	Published - Jul 2012

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

planetary systems
stars: individual (HAT-P-34, GSC 1622-01261, HAT-P-35, GSC 0203-01079, HAT-P-36, ⋯ ⋯)
techniques: photometric
techniques: spectroscopic

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Bakos, G. Á., Hartman, J. D., Torres, G., Béky, B., Latham, D. W., Buchhave, L. A., Csubry, Z., Kovács, G., Bieryla, A., Quinn, S., Szklenár, T., Esquerdo, G. A., Shporer, A., Noyes, R. W., Fischer, D. A., Johnson, J. A., Howard, A. W., Marcy, G. W., Sato, B., ... Sári, P. (2012). HAT-P-34b-HAT-P-37b: Four transiting planets more massive than Jupiter orbiting moderately bright stars. Astronomical Journal, 144(1), Article 19. https://doi.org/10.1088/0004-6256/144/1/19

@article{dac962f790f444c891a40c8e40ca5661,

title = "HAT-P-34b-HAT-P-37b: Four transiting planets more massive than Jupiter orbiting moderately bright stars",

abstract = "We report the discovery of four transiting extrasolar planets (HAT-P-34b-HAT-P-37b) with masses ranging from 1.05 to 3.33M J and periods from 1.33 to 5.45days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33M J), has a high eccentricity of e = 0.441 ± 0.032 at a period of P = 5.452654 ± 0.000016 days, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.",

keywords = "planetary systems, stars: individual (HAT-P-34, GSC 1622-01261, HAT-P-35, GSC 0203-01079, HAT-P-36, ⋯ ⋯), techniques: photometric, techniques: spectroscopic",

author = "Bakos, {G. {\'A}} and Hartman, {J. D.} and G. Torres and B. B{\'e}ky and Latham, {D. W.} and Buchhave, {L. A.} and Z. Csubry and G. Kov{\'a}cs and A. Bieryla and S. Quinn and T. Szklen{\'a}r and Esquerdo, {G. A.} and A. Shporer and Noyes, {R. W.} and Fischer, {D. A.} and Johnson, {J. A.} and Howard, {A. W.} and Marcy, {G. W.} and B. Sato and K. Penev and M. Everett 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 = jul,

doi = "10.1088/0004-6256/144/1/19",

language = "English (US)",

volume = "144",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "1",

}

Bakos, GÁ , Hartman, JD, Torres, G, Béky, B, Latham, DW, Buchhave, LA, Csubry, Z, Kovács, G, Bieryla, A, Quinn, S, Szklenár, T, Esquerdo, GA, Shporer, A, Noyes, RW, Fischer, DA, Johnson, JA, Howard, AW, Marcy, GW, Sato, B, Penev, K, Everett, M, Sasselov, DD, Frész, G, Stefanik, RP, Lázár, J, Papp, I & Sári, P 2012, 'HAT-P-34b-HAT-P-37b: Four transiting planets more massive than Jupiter orbiting moderately bright stars', Astronomical Journal, vol. 144, no. 1, 19. https://doi.org/10.1088/0004-6256/144/1/19

TY - JOUR

T1 - HAT-P-34b-HAT-P-37b

T2 - Four transiting planets more massive than Jupiter orbiting moderately bright stars

AU - Bakos, G. Á

AU - Hartman, J. D.

AU - Torres, G.

AU - Béky, B.

AU - Latham, D. W.

AU - Buchhave, L. A.

AU - Csubry, Z.

AU - Kovács, G.

AU - Bieryla, A.

AU - Quinn, S.

AU - Szklenár, T.

AU - Esquerdo, G. A.

AU - Shporer, A.

AU - Noyes, R. W.

AU - Fischer, D. A.

AU - Johnson, J. A.

AU - Howard, A. W.

AU - Marcy, G. W.

AU - Sato, B.

AU - Penev, K.

AU - Everett, M.

AU - Sasselov, D. D.

AU - Frész, G.

AU - Stefanik, R. P.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2012/7

Y1 - 2012/7

N2 - We report the discovery of four transiting extrasolar planets (HAT-P-34b-HAT-P-37b) with masses ranging from 1.05 to 3.33M J and periods from 1.33 to 5.45days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33M J), has a high eccentricity of e = 0.441 ± 0.032 at a period of P = 5.452654 ± 0.000016 days, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.

AB - We report the discovery of four transiting extrasolar planets (HAT-P-34b-HAT-P-37b) with masses ranging from 1.05 to 3.33M J and periods from 1.33 to 5.45days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33M J), has a high eccentricity of e = 0.441 ± 0.032 at a period of P = 5.452654 ± 0.000016 days, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.

KW - planetary systems

KW - stars: individual (HAT-P-34, GSC 1622-01261, HAT-P-35, GSC 0203-01079, HAT-P-36, ⋯ ⋯)

KW - techniques: photometric

KW - techniques: spectroscopic

UR - http://www.scopus.com/inward/record.url?scp=84862509055&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84862509055&partnerID=8YFLogxK

U2 - 10.1088/0004-6256/144/1/19

DO - 10.1088/0004-6256/144/1/19

M3 - Article

AN - SCOPUS:84862509055

SN - 0004-6256

VL - 144

JO - Astronomical Journal

JF - Astronomical Journal

IS - 1

M1 - 19

ER -

HAT-P-34b-HAT-P-37b: Four transiting planets more massive than Jupiter orbiting moderately bright stars

Abstract

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