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Examining the broadband emission spectrum of WASP-19b: A new z-band eclipse detection

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dc.contributor.authorZhou, Yan Jun (George)
dc.contributor.authorKedziora-Chudczer, Lucyna L.
dc.contributor.authorBayliss, Daniel
dc.contributor.authorBailey, J
dc.date.accessioned2015-12-13T22:27:12Z
dc.date.issued2013
dc.date.updated2016-02-24T09:18:12Z
dc.description.abstractWASP-19b is one of the most irradiated hot-Jupiters known. Its secondary eclipse is the deepest of all transiting planets and has been measured in multiple optical and infrared bands. We obtained a z-band eclipse observation with a measured depth of 0.080
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/73842
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: planets and satellites: atmospheres; planets and satellites: individual (WASP-19b)
dc.titleExamining the broadband emission spectrum of WASP-19b: A new z-band eclipse detection
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.startpage8
local.contributor.affiliationZhou, Yan Jun (George), College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKedziora-Chudczer, Lucyna L., University of New South Wales
local.contributor.affiliationBayliss, Daniel, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBailey, J, University of New South Wales
local.contributor.authoruidZhou, Yan Jun (George), u4530806
local.contributor.authoruidBayliss, Daniel, u4102644
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB3855
local.identifier.citationvolume774
local.identifier.doi10.1088/0004-637X/774/2/118
local.identifier.scopusID2-s2.0-84883634885
local.identifier.thomsonID000323888900027
local.type.statusPublished Version

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