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dc.contributor.authorBarnes, J.R.
dc.contributor.authorLeigh, C.J.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorBarman, T.S.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorCollier Cameron, A.
dc.contributor.authorJenkins, J.S.
dc.date.accessioned2008-02-01T11:41:23Z
dc.date.available2008-02-01T11:41:23Z
dc.date.issued2007
dc.identifier.citationBarnes , J R , Leigh , C J , Jones , H R A , Barman , T S , Pinfield , D J , Collier Cameron , A & Jenkins , J S 2007 , ' Near infrared spectroscopic search for the close orbiting planet HD 75289b ' , Monthly Notices of the Royal Astronomical Society , vol. 379 , no. 3 , pp. 1097-1107 . https://doi.org/10.1111/j.1365-2966.2007.11990.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 144513
dc.identifier.otherPURE UUID: 9c7b4686-aaf8-45fa-964f-af060169c2ad
dc.identifier.otherdspace: 2299/1519
dc.identifier.otherScopus: 34547507026
dc.identifier.urihttp://hdl.handle.net/2299/1519
dc.descriptionThe definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing DOI : 10.1111/j.1365-2966.2007.11990.x
dc.description.abstractWe present a search for the near infrared spectroscopic signature of the close orbiting extrasolar giant planet HD 75289b. We obtained »230 spectra in the wavelength range 2.18 ¹m- 2.19 ¹m using the Phoenix spectrograph at Gemini South. By considering the direct spectrum, derived from irradiated model atmospheres, we search for the absorption profile signature present in the combined star and planet light. Since the planetary spectrum is separated from the stellar spectrum at most phases, we apply a phase dependent orbital model and tomographic techniques to search for absorption signatures.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.titleNear infrared spectroscopic search for the close orbiting planet HD 75289ben
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2007
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2007.11990.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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