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HATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars

Author(s): Bento, J; Hartman, JD; Bakos, Gaspar Aron; Bhatti, W; Csubry, Z; et al

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dc.contributor.authorBento, J-
dc.contributor.authorHartman, JD-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorBhatti, W-
dc.contributor.authorCsubry, Z-
dc.contributor.authorPenev, K-
dc.contributor.authorBayliss, D-
dc.contributor.authorde Val-Borro, M-
dc.contributor.authorZhou, G-
dc.contributor.authorBrahm, R-
dc.contributor.authorEspinoza, N-
dc.contributor.authorRabus, M-
dc.contributor.authorJordan, A-
dc.contributor.authorSuc, V-
dc.contributor.authorCiceri, S-
dc.contributor.authorSarkis, P-
dc.contributor.authorHenning, T-
dc.contributor.authorMancini, L-
dc.contributor.authorTinney, CG-
dc.contributor.authorWright, DJ-
dc.contributor.authorDurkan, S-
dc.contributor.authorTan, TG-
dc.contributor.authorLazar, J-
dc.contributor.authorPapp, I-
dc.contributor.authorSari, P-
dc.date.accessioned2019-04-10T19:32:14Z-
dc.date.available2019-04-10T19:32:14Z-
dc.date.issued2018-07en_US
dc.identifier.citationBento, J, Hartman, JD, Bakos, GA, Bhatti, W, Csubry, Z, Penev, K, Bayliss, D, de Val-Borro, M, Zhou, G, Brahm, R, Espinoza, N, Rabus, M, Jordan, A, Suc, V, Ciceri, S, Sarkis, P, Henning, T, Mancini, L, Tinney, CG, Wright, DJ, Durkan, S, Tan, TG, Lazar, J, Papp, I, Sari, P. (2018). HATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 477 (3406 - 3423. doi:10.1093/mnras/sty726en_US
dc.identifier.issn0035-8711-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1bh85-
dc.description.abstractWe report the discovery of four transiting hot Jupiters from the HATSouth survey: HATS39b, HATS-40b, HATS-41b, and HATS-42b. These discoveries add to the growing number of transiting planets orbiting moderately bright (12.5 less than or similar to V less than or similar to 13.7) F dwarf stars on short (2-5 d) periods. The planets have similar radii, ranging from 1.33(+0.29) (-0.20) RJ for HATS- 41b to 1.58(+0.16) (-0.12) RJ for HATS-40b. Their masses and bulk densities, however, span more than an order of magnitude. HATS-39b has a mass of 0.63 +/- 0.13M(J), and an inflated radius of 1.57 +/- 0.12 R-J, making it a good target for future transmission spectroscopic studies. HATS41b is a very massive 9.7 +/- 1.6M(J) planet and one of only a few hot Jupiters found to date with a mass over 5 M-J. This planet orbits the highest metallicity star ([Fe/H] = 0.470 +/- 0.010) known to host a transiting planet and is also likely on an eccentric orbit. The highmass, coupled with a relatively young age (1.34(+0.31) (-0.51) Gyr) for the host star, is a factor that may explain why this planet’s orbit has not yet circularized.en_US
dc.format.extent3406 - 3423en_US
dc.languageEnglishen_US
dc.language.isoen_USen_US
dc.relation.ispartofMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleHATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F starsen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1093/mnras/sty726-
dc.date.eissued2018-03-20en_US
dc.identifier.eissn1365-2966-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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