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dc.contributor.authorLyubchik, Y.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorPavlenko, Y.
dc.contributor.authorViti, S.
dc.contributor.authorPickering, J.C.
dc.contributor.authorBlackwell-Whitehead, R.J.
dc.date.accessioned2007-07-08T20:14:19Z
dc.date.available2007-07-08T20:14:19Z
dc.date.issued2004-03
dc.identifier.citationLyubchik , Y , Jones , H R A , Pavlenko , Y , Viti , S , Pickering , J C & Blackwell-Whitehead , R J 2004 , ' Atomic lines in infrared spectra for ultracool dwarfs ' , Astronomy and Astrophysics , vol. 416 , pp. 655-659 .
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 162798
dc.identifier.otherPURE UUID: 91665ed6-cb65-4abd-8d17-7ab20cc0230b
dc.identifier.otherdspace: 2299/166
dc.identifier.otherScopus: 1642296621
dc.identifier.urihttp://hdl.handle.net/2299/166
dc.description.abstractWe provide a set of atomic lines which are suitable for the description of ultracool dwarf spectra from 10 000 to 25 000 Å. This atomic linelist was made using both synthetic spectra calculations and existing atlases of infrared spectra of Arcturus and Sunspot umbra. We present plots which show the comparison of synthetic spectra and observed Arcturus and Sunspot umbral spectra for all atomic lines likely to be observable in high resolution infrared spectra.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.titleAtomic lines in infrared spectra for ultracool dwarfsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre of Data Innovation Research
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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