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dc.contributor.authorBento, J.
dc.contributor.authorHartman, J. D.
dc.contributor.authorBakos, G. A.
dc.contributor.authorBhatti, W.
dc.contributor.authorCsubry, Z.
dc.contributor.authorPenev, Kaloyan
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, C. G.
dc.contributor.authorWright, D. J.
dc.contributor.authorDurkan, S.
dc.contributor.authorTan, T. G.
dc.contributor.authorLazar, J.
dc.contributor.authorPapp, I.
dc.contributor.authorSari, P.
dc.date.accessioned2019-07-26T17:39:38Z
dc.date.available2019-07-26T17:39:38Z
dc.date.created2018-03-20
dc.identifier.issn0035-8711
dc.identifier.urihttps://hdl.handle.net/10735.1/6752
dc.descriptionFull text access from Treasures at UT Dallas is restricted to current UTD affiliates (use the provided Link to Article). Non UTD affiliates will find the web address for this item by clicking the "Show full item record" link, copying the "dc.relation.uri" metadata and pasting it into a browser.
dc.descriptionIncludes supplementary material
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 ≲ V ≲ 13.7) F dwarf stars on short (2-5 d) periods. The planets have similar radii, ranging from 1.33{_{0.20}^{+0.29}} R_J for HATS-41b to 1.58{_{-0.12} ^{+0.16}} R_J 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 high mass, coupled with a relatively young age (1.34{_{-0.51} ^{+0.31}} Gyr) for the host star, is a factor that may explain why this planet's orbit has not yet circularized.
dc.description.sponsorshipNSF MRI grant NSF/AST-0723074, 1108686; NASA grants NNX09AB29G, NNX12AH91H, NNX14AE87G and NNX17AB61G; FONDECYT project 1171208; BASAL CATA PFB-06; ARC Laureate Fellowship Grant FL0992131; European Organization for Astronomical Research in the Southern hemisphere programmes 095.C-0367, CN2013A-171, CN2013B-55, CN2014A-104, CN2014B-57, CN2015A-51, and ESO 096.C-0544.
dc.language.isoen
dc.publisherOxford Univ Press
dc.relation.urihttp://dx.doi.org/10.1093/mnras/sty726
dc.rights©2018 The Authors
dc.subjectKepler's laws
dc.subjectTelescopes
dc.subjectPhotometry--Techniques
dc.subjectAstronomical spectroscopy
dc.subjectStars
dc.subjectPlanetary systems
dc.titleHATS-39b, HATS-40b, HATS-41b, and HATS-42b: Three Inflated Hot Jupiters and a Super-Jupiter Transiting F Stars
dc.type.genrearticle
dc.description.departmentSchool of Natural Sciences and Mathematics
dc.identifier.bibliographicCitationBento, J., J. D. Hartman, G. A. Bakos, W. Bhatti, et al. 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(3): 3406-3423, doi:10.1093/mnras/sty726
dc.source.journalMonthly Notices of the Royal Astronomical Society
dc.identifier.volume477
dc.identifier.issue3
dc.contributor.utdAuthorPenev, Kaloyan
dc.contributor.ORCID0000-0003-4464-1371 (Penev, K)


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