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HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity

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dc.contributor.authorMohler-Fischer, M.
dc.contributor.authorMancini, L.
dc.contributor.authorHartman, J.
dc.contributor.authorBakos, Gaspar
dc.contributor.authorPenev, K.
dc.contributor.authorBayliss, Daniel
dc.contributor.authorJordan, A.
dc.contributor.authorCsubry, Z.
dc.contributor.authorRabus, M.
dc.contributor.authorNikolov, N.
dc.contributor.authorZhou, Guyin (George)
dc.contributor.authorBrahm, R.
dc.contributor.authorEspinoza, N.
dc.contributor.authorBuchhave, L. A.
dc.contributor.authorBeky, B.
dc.contributor.authorSuc, V.
dc.contributor.authorSchmidt, Brian
dc.contributor.authorConroy, Peter
dc.date.accessioned2015-12-13T22:39:27Z
dc.date.issued2013
dc.date.updated2016-02-24T09:30:19Z
dc.description.abstractWe report the discovery of HATS-2b, the second transiting extrasolar planet detected by the HATSouth survey. HATS-2b is moving on a circular orbit around a V = 13.6 mag, K-type dwarf star (GSC 6665-00236), at a separation of 0.0230 ± 0.0003 AU and with a
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 receive partial support from grant NSF/AST-1108686. A.J. acknowledges support from Fondecyt project 1130857, Anillo ACT-086, BASAL CATA PFB-06 and the Millenium Science Initiative, Chilean Ministry of Economy (Nucleus P10-022-F). V.S. acknowledges support form BASAL CATA PFB-06. R.B. and N.E. acknowledge support from Fondecyt project 1095213. N.N. acknowledges support from an STFC consolidated grant. M.R. acknowledges support from a FONDECYT postdoctoral fellowship N03120097. 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 the CDS, Strasbourg, France. Work at UNSW has been supported by ARC Australian Professorial Fellowship grant DP0774000, ARC LIEF grant LE0989347 and ARC Super Science Fellowships FS100100046.
dc.format13 pages
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/77791
dc.provenancehttp://www.sherpa.ac.uk/romeo/issn/0004-6361/ Author can archive publisher's version/PDF. On author's personal website or institutional website or OAI compliant website (Sherpa/Romeo as of 26/9/2018).
dc.publisherSpringer
dc.relationhttp://purl.org/au-research/grants/arc/FL110100012
dc.rights© ESO 2013en_AU
dc.sourceAstronomy and Astrophysics
dc.subjectPlanetary system
dc.subjectStars: individual
dc.subjectStars: fundamental parameters
dc.subjectTechniques: photometric
dc.subjectTechniques: spectroscopic
dc.subjectExtrasolar planets
dc.subjectPhotometry
dc.subjectStars Planetary systems
dc.subjectStars: fundamental parameters
dc.subjectStars: individual: GSC 6665-00236
dc.subjectStars: individual: HATS-2
dc.subjectTechniques: photometric
dc.subjectTechniques: spectroscopic
dc.titleHATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage13
local.bibliographicCitation.startpage1
local.contributor.affiliationMohler-Fischer, M, Max Planck Institute for Astronomy
local.contributor.affiliationMancini, L, Max Planck Institute for Astronomy
local.contributor.affiliationHartman, J, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationBakos, Gaspar, Harvard Smithsonian Center for Astrophysics
local.contributor.affiliationPenev , K, 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.affiliationCsubry, Z, Princeton University
local.contributor.affiliationRabus, M, Pontificia Universidad Catolica de Chile
local.contributor.affiliationNikolov, N, University of Exeter
local.contributor.affiliationZhou, Guyin (George), College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationBrahm, R, Pontificia Universidad Catolica de Chile
local.contributor.affiliationEspinoza, N, Pontificia Universidad Catolica de Chile
local.contributor.affiliationBuchhave, L. A. , Copenhagen University
local.contributor.affiliationBeky, B, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationSuc, V, Pontificia Universidad Catolica de Chile
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationConroy, Peter, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.authoruidBayliss, Daniel, u4102644
local.contributor.authoruidZhou, Guyin (George), u3932441
local.contributor.authoruidSchmidt, Brian, u9500253
local.contributor.authoruidConroy, Peter, u7200280
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB6571
local.identifier.citationvolume558
local.identifier.doi10.1051/0004-6361/201321663
local.identifier.essn1432-0746
local.identifier.scopusID2-s2.0-84885089744
local.identifier.thomsonID000326574000055
local.type.statusPublished Version

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