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The mass-radius relationship for very low mass stars: Four new discoveries from the HATSouth Survey

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dc.contributor.authorZhou, Guyin (George)
dc.contributor.authorBayliss, Daniel
dc.contributor.authorHartman, J. D.
dc.contributor.authorBakos, Gaspar
dc.contributor.authorPenev, K.
dc.contributor.authorCsubry, Z.
dc.contributor.authorMancini, L.
dc.contributor.authorMohler-Fischer, M.
dc.contributor.authorCiceri, Simona
dc.contributor.authorSchmidt, Brian
dc.date.accessioned2015-12-13T22:38:01Z
dc.date.issued2014
dc.date.updated2015-12-11T09:39:58Z
dc.description.abstractWe report the discovery of four transiting F-M binary systems with companions between 0.1 and 0.2M⊙ in mass by the HATSouth survey. These systems have been characterized via a global analysis of the HATSouth discovery data, combined with high-resolution
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. Work at the Australian National University is supported by ARC Laureate Fellowship Grant FL0992131. Follow-up observations with the ESO 2.2 m/FEROS instrument were performed under MPI guaranteed time [P087.A9014(A), P088.A-9008(A), P089.A-9008(A)]. AJ acknowledges support from FONDECYT project 1130857, BASAL CATA PFB06 and the Millenium Science Initiative, Chilean Ministry of Economy (Nuclei: P10-022-F, P07-021-F). RB and NE are supported by CONICYT-PCHA/Doctorado Nacional and MR is supported by FONDECYT postdoctoral fellowship 3120097. We acknowledge the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund, and the SIMBAD data base, operated at CDS, Strasbourg, France. Operations at the MPG/ESO 2.2 m telescope are jointly performed by the Max Planck Gesellschaft and the European Southern Observatory.
dc.format14 pages
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/77358
dc.provenancehttp://www.sherpa.ac.uk/romeo/issn/0035-8711/ Author can archive publisher's version/PDF. Publisher's version/PDF on Institutional repositories or Central repositories, with all rights reserved (Sherpa/Romeo as of 17/10/2018)
dc.publisherBlackwell Publishing Ltd
dc.relationhttp://purl.org/au-research/grants/arc/FL0992131.
dc.relationhttp://purl.org/au-research/grants/arc/FL0992131
dc.rights© 2013 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. https://academic.oup.com/journals/pages/access_purchase/rights_and_permissions/self_archiving_policy_p This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©:2013 G. Zhou D. Bayliss J. D. Hartman G. Á. Bakos K. Penev Z. Csubry T. G. Tan A. Jordán L. Mancini M. Rabus R. Brahm N. Espinoza M. Mohler-Fischer S. Ciceri V. Suc B. Csák T. Henning B. Schmidt. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. (Publisher journal website as of 17/10/2018).en_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.titleThe mass-radius relationship for very low mass stars: Four new discoveries from the HATSouth Survey
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage2844
local.bibliographicCitation.startpage2831
local.contributor.affiliationZhou, Guyin (George), College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationBayliss, Daniel, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationHartman, J D, Princeton University
local.contributor.affiliationBakos, Gaspar, Harvard Smithsonian Center for Astrophysics
local.contributor.affiliationPenev , K, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationCsubry, Z, Princeton University
local.contributor.affiliationMancini, L, Max Planck Institute for Astronomy
local.contributor.affiliationMohler-Fischer, M, Max Planck Institute for Astronomy
local.contributor.affiliationCiceri, Simona, Max Planck Institut fur Astronomie
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.authoruidZhou, Guyin (George), u3932441
local.contributor.authoruidBayliss, Daniel, u4102644
local.contributor.authoruidSchmidt, Brian, u9500253
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB6231
local.identifier.citationvolume437
local.identifier.doi10.1093/mnras/stt2100
local.identifier.essn1365-2966
local.identifier.scopusID2-s2.0-84891369910
local.identifier.thomsonID000329158900062
local.type.statusPublished Version

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