HATS-1b: The first transiting planet discovered by the hatsouth survey

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dc.contributor.authorPenev, K.
dc.contributor.authorBakos, Gaspar
dc.contributor.authorBayliss, Daniel
dc.contributor.authorJordan, A.
dc.contributor.authorMohler-Fischer, M.
dc.contributor.authorZhou, Guyin (George)
dc.contributor.authorSuc, V.
dc.contributor.authorRabus, M.
dc.contributor.authorHartman, J.
dc.contributor.authorMancini, L.
dc.contributor.authorConroy, Peter
dc.contributor.authorSchmidt, Brian
dc.contributor.authorWright, D. J.
dc.contributor.authorTinney, C. G.
dc.contributor.authorMohler, Maren
dc.date.accessioned2015-12-13T23:01:45Z
dc.date.issued2013
dc.date.updated2016-02-24T08:42:56Z
dc.description.abstractWe report the discovery of HATS-1b, a transiting extrasolar planet orbiting the moderately bright V = 12.05 G dwarf star GSC 6652-00186, and the first planet discovered by HATSouth, a global network of autonomous wide-field telescopes. HATS-1b has a period of P ≈ 3.4465 days, mass of Mp ≈ 1.86 MJ, and radius of Rp ≈ 1.30 RJ. The host star has a mass of 0.99 M⊙ and radius of 1.04 R⊙. The discovery light curve of HATS-1b has near-continuous coverage over several multi-day timespans, demonstrating the power of using a global network of telescopes to discover transiting planets.
dc.description.sponsorshipDevelopment of the HATSouth project was funded by NSF MRI grant NSF/AST-0723074, operations are supported by NASA grant NNX09AB29G, and follow-up observations received partial support from grant NSF/AST-1108686. Followup observations with the ESO 2.2 m/FEROS instrument were performed under MPI guaranteed time (P087.A-9014(A), P088.A-9008(A), P089.A-9008(A)) and Chilean time (P087.C- 0508(A)). A.J. acknowledges support from Fondecyt project 1095213, Ministry of Economy ICM Nuclei P07-021-F and P10-022-F, Anillo ACT-086 and BASAL CATA PFB-06. V.S. acknowledges support form BASAL CATA PFB-06. M.R. acknowledges support from a Fondencyt postdoctoral fellowship N 3120097 and contributions from the ALMA-CONICYT FUND Project N 31090015. R.B. and N.E. acknowledge support from Fondecyt project 1095213. Work at the Australian National University is supported by ARC Laureate Fellowship Grant FL0992131. We acknowledge the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund, and the SIMBAD database, operated at CDS, Strasbourg, France.
dc.format11 pages
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/84567
dc.provenancehttp://www.sherpa.ac.uk/romeo/issn/0004-6256/ Author can archive publisher's version/PDF. Publisher's version/PDF may be used on any website or authors' institutional repository (Sherpa/Romeo as of 26/9/2018).
dc.publisherUniversity of Chicago Press
dc.relationhttp://purl.org/au-research/grants/arc/FL0992131
dc.rights© 2013. The American Astronomical Society. Author/s retain copyright.en_AU
dc.sourceAstronomical Journal
dc.subjectKeywords: planetary systems; stars: individual (HATS-1, GSC 6652-00186); techniques: photometric; techniques: spectroscopic
dc.titleHATS-1b: The first transiting planet discovered by the hatsouth survey
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage11
local.bibliographicCitation.startpage1
local.contributor.affiliationPenev , K, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationBakos, Gaspar, Harvard Smithsonian Center for Astrophysics
local.contributor.affiliationBayliss, Daniel, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationJordan, A, Pontificia Universidad Catolica de Chile
local.contributor.affiliationMohler-Fischer, M, Max Planck Institute for Astronomy
local.contributor.affiliationZhou, Guyin (George), College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationSuc, V, Pontificia Universidad Catolica de Chile
local.contributor.affiliationRabus, M, Pontificia Universidad Catolica de Chile
local.contributor.affiliationHartman, J, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationMancini, L, Max Planck Institute for Astronomy
local.contributor.affiliationConroy, Peter, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationWright, D. J., University of New South Wales
local.contributor.affiliationTinney, C. G., University of New South Wales
local.contributor.affiliationMohler, Maren, Max Planck Institut fur Astronomie
local.contributor.authoremailu7200280@anu.edu.au
local.contributor.authoruidBayliss, Daniel, u4102644
local.contributor.authoruidZhou, Guyin (George), u3932441
local.contributor.authoruidConroy, Peter, u7200280
local.contributor.authoruidSchmidt, Brian, u9500253
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB12854
local.identifier.citationvolume145
local.identifier.doi10.1088/0004-6256/145/1/5
local.identifier.essn1538-3881
local.identifier.scopusID2-s2.0-84870178699
local.identifier.thomsonID000312251100005
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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