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dc.contributor.authorRogers, Justin C.
dc.contributor.authorApai, Daniel
dc.contributor.authorLopez-Morales, M.
dc.contributor.authorSing, David K.
dc.contributor.authorBurrows, A.S.
dc.date.accessioned2014-12-18T11:32:38Z
dc.date.issued2010-10-26
dc.description.abstractWe discovered a typographical error in the program we used for modeling CoRoT-1b as a blackbody. While correcting this error slightly changes two of the figures, the changes to most parameters were within the error bars. The error did not affect the comparison to the more realistic planetary atmosphere models and the conclusions of the paper.en_GB
dc.description.sponsorshipSpace Telescope Science Instituteen_GB
dc.description.sponsorshipNASA - Hubble Fellowship grant (awarded by the STScI)en_GB
dc.description.sponsorshipCNESen_GB
dc.description.sponsorshipNASAen_GB
dc.description.sponsorshipNational Science Foundationen_GB
dc.identifier.citationVol. 723 (2), pp. 1825 - 1826en_GB
dc.identifier.doi10.1088/0004-637X/723/2/1825
dc.identifier.grantnumberD0101.90131en_GB
dc.identifier.grantnumberHF-01210.01-Aen_GB
dc.identifier.grantnumberNNX07AG80Gen_GB
dc.identifier.grantnumberAST–0908278en_GB
dc.identifier.urihttp://hdl.handle.net/10871/16088
dc.language.isoen_USen_GB
dc.publisherIOP Publishing for American Astronomical Societyen_GB
dc.relation.urihttp://hdl.handle.net/10871/16081
dc.relation.urlhttp://hdl.handle.net/10871/16081
dc.rightsCopyright © 2010 IOP Publishing / American Astronomical Society
dc.subjectbinaries: eclipsingen_GB
dc.subjectplanetary systemsen_GB
dc.subjectstars: individual (CoRoT-1)en_GB
dc.subjecttechniques: photometricen_GB
dc.subjectErrata, addendaen_GB
dc.titleErratum: Ks-Band Detection of Thermal Emission and Color Constraints to CoRoT-1b: A Low-Albedo Planet with Inefficient Atmospheric Energy Redistribution and a Temperature Inversionen_GB
dc.typeArticleen_GB
dc.date.available2014-12-18T11:32:38Z
dc.identifier.issn0004-637X
pubs.declined2014-12-15T10:36:52.588+0000
dc.descriptionThis is an erratum for the article published in the Astrophysical Journal Vol. 707 (2), pp. 1707-1716. DOI: 10.1088/0004-637X/707/2/1707en_GB
dc.descriptionSee the ORE record http://hdl.handle.net/10871/16081 for the original articleen_GB
dc.identifier.eissn1538-4357
dc.identifier.journalAstrophysical Journalen_GB


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