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The Frequency of Large-Radius Hot and Very Hot Jupiters in ω Centauri

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dc.contributor.authorWeldrake, David
dc.contributor.authorSackett, Penny
dc.contributor.authorBridges, Terry C
dc.date.accessioned2015-12-08T22:20:32Z
dc.date.issued2008
dc.date.updated2015-12-08T08:31:22Z
dc.description.abstractWe present the results of a deep, wide-field search for transiting hot Jupiter (HJ) planets in the globular cluster ω Centauri. As a result of a 25 night observing run with the ANU 40 inch (1 m) telescope at Siding Spring Observatory, a total of 109,726
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/32045
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Globular clusters: individual (NGC 5139, ? Centauri); Planetary systems; Techniques: photometric
dc.titleThe Frequency of Large-Radius Hot and Very Hot Jupiters in ω Centauri
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1129
local.bibliographicCitation.startpage1117
local.contributor.affiliationWeldrake, David, Max Plank Institute for Astronomy
local.contributor.affiliationSackett, Penny, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBridges, Terry C, Queen's University
local.contributor.authoruidSackett, Penny, u4049146
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020108 - Planetary Science (excl. Extraterrestrial Geology)
local.identifier.ariespublicationu4362859xPUB88
local.identifier.citationvolume674
local.identifier.doi10.1086/524917
local.identifier.scopusID2-s2.0-40249099198
local.identifier.thomsonID000253454500037
local.type.statusPublished Version

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