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dc.contributor.authorHuang, Chelsea
dc.contributor.authorShporer, Avi
dc.contributor.authorRicker, George R.
dc.contributor.authorVanderspek, Roland K.
dc.contributor.authorSeager, Sara
dc.contributor.authorGoeke, Robert F.
dc.contributor.authorGuerrero, Natalia
dc.contributor.authorVillanueva, Steven
dc.date.accessioned2020-04-17T17:58:49Z
dc.date.available2020-04-17T17:58:49Z
dc.date.issued2019-10
dc.date.submitted2019-06
dc.identifier.issn1538-3881
dc.identifier.urihttps://hdl.handle.net/1721.1/124729
dc.description.abstractWide-field surveys for transiting planets are well suited to searching diverse stellar populations, enabling a better understanding of the link between the properties of planets and their parent stars. We report the discovery of HAT-P-69 b (TOI 625.01) and HAT-P-70 b (TOI 624.01), two new hot Jupiters around A stars from the Hungarian-made Automated Telescope Network (HATNet) survey that have also been observed by the Transiting Exoplanet Survey Satellite. HAT-P-69 b has a mass of M Jup and a radius of $ R Jup and resides in a prograde 4.79 day orbit. HAT-P-70 b has a radius of R Jup and a mass constraint of M Jup and resides in a retrograde 2.74 day orbit. We use the confirmation of these planets around relatively massive stars as an opportunity to explore the occurrence rate of hot Jupiters as a function of stellar mass. We define a sample of 47,126 main-sequence stars brighter than T mag = 10 that yields 31 giant planet candidates, including 18 confirmed planets, 3 candidates, and 10 false positives. We find a net hot Jupiter occurrence rate of 0.41 0.10% within this sample, consistent with the rate measured by Kepler for FGK stars. When divided into stellar mass bins, we find the occurrence rate to be 0.71 0.31% for G stars, 0.43 0.15% for F stars, and 0.26 0.11% for A stars. Thus, at this point, we cannot discern any statistically significant trend in the occurrence of hot Jupiters with stellar mass. ©2019en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/1538-3881/AB36B5en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceThe American Astronomical Societyen_US
dc.titleTwo new HATNet hot Jupiters around A stars and the first glimpse at the occurrence rate of hot Jupiters from TESSen_US
dc.typeArticleen_US
dc.identifier.citationZhou, G., et al., "Two new HATNet hot Jupiters around A stars and the first glimpse at the occurrence rate of hot Jupiters from TESS." Astronomical journal 158, 4 (October 2019): no. 141 doi 10.3847/1538-3881/AB36B5 ©2019 Author(s)en_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.relation.journalAstronomical journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2020-04-09T14:42:38Z
dspace.orderedauthorsG. Zhou ; Huang, Chelsea ; G. Á. Bakos ; J. D. Hartman ; David W. Latham ; S. N. Quinn ; K. A. Collins ; J. N. Winn ; I. Wong ; G. Kovács ; Z. Csubry ; W. Bhatti ; K. Penev ; A. Bieryla ; G. A. Esquerdo ; P. Berlind ; M. L. Calkins ; M. de Val-Borro ; R. W. Noyes ; J. Lázár ; I. Papp ; P. Sári ; T. Kovács ; Lars A. Buchhave ; T. Szklenar ; B. Béky ; M. C. Johnson ; W. D. Cochran ; A. Y. Kniazev ; K. G. Stassun ; B. J. Fulton ; Shporer, Avi ; N. Espinoza ; D. Bayliss ; M. Everett ; S. B. Howell ; C. Hellier ; D. R. Anderson ; A. Collier Cameron ; R. G. West ; D. J. A. Brown ; N. Schanche ; K. Barkaoui ; F. Pozuelos ; M. Gillon ; E. Jehin ; Z. Benkhaldoun ; A. Daassou ; Ricker, George R. ; Vanderspek, Roland K. ; Seager, Sara ; J. M. Jenkins ; Jack J. Lissauer ; J. D. Armstrong ; K. I. Collins ; T. Gan ; R. Hart ; K. Horne ; J. F. Kielkopf ; L. D. Nielsen ; T. Nishiumi ; N. Narita ; E. Palle ; H. M. Relles ; R. Sefako ; T. G. Tan ; M. Davies ; Goeke, Robert F. ; Guerrero, Natalia ; K. Haworth ; Villanueva, Stevenen_US
dspace.date.submission2020-04-09T14:43:00Z
mit.journal.volume158en_US
mit.journal.issue4en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusComplete


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