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dc.contributor.authorRamsey, L.
dc.contributor.authorBarnes, John
dc.contributor.authorRedman, S.L.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorWolscznan, A.
dc.contributor.authorBongiorno, S.
dc.contributor.authorEngel, L.
dc.contributor.authorJenkins, J.S.
dc.date.accessioned2011-08-17T14:01:06Z
dc.date.available2011-08-17T14:01:06Z
dc.date.issued2008
dc.identifier.citationRamsey , L , Barnes , J , Redman , S L , Jones , H R A , Wolscznan , A , Bongiorno , S , Engel , L & Jenkins , J S 2008 , ' A pathfinder instrument for precision radial velocities in the near-infrared ' , Publications of the Astronomical Society of the Pacific , vol. 120 , no. 870 , pp. 887-894 . https://doi.org/10.1086/591233
dc.identifier.issn0004-6280
dc.identifier.urihttp://hdl.handle.net/2299/6285
dc.descriptionOriginal article can be found at : http://www.journals.uchicago.edu/ Copyright Astronomical Society of the Pacific
dc.description.abstractWe have designed and tested an in-plane echelle spectrograph configured to investigate precision radial velocities from ground-based near-infrared observations. The spectrograph operates across the spectral range of 0.9–1.7 μm at a spectral resolution of R ¼ 50; 000, and uses a liquid nitrogen-cooled HAWAII 1 K detector. Repeated measurements of the Earth’s rotation via integrated sunlight with two different instrument arrangements in the near-infrared Y band have produced radial velocities with ∼10 ms1 rms over a period of several hours. The most recent instrument configuration has achieved an unbinned rms of 7 ms1 and suggests that infrared radial velocity precisions may be able to approach those achieved at optical wavelengths.en
dc.format.extent567286
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacific
dc.subjectastronomical instrumentation
dc.titleA pathfinder instrument for precision radial velocities in the near-infrareden
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1086/591233
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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