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dc.contributor.authorJones, H.R.A.
dc.contributor.authorRayer, J.
dc.contributor.authorRamsey, L.
dc.contributor.authorDent, B.
dc.contributor.authorLongmore, A.J.
dc.contributor.authorVacva, B.
dc.contributor.authorLiu, M.
dc.contributor.authorWebster, A.
dc.contributor.authorWolscznan, A.
dc.contributor.authorBarnes, A.
dc.identifier.citationJones , H R A , Rayer , J , Ramsey , L , Dent , B , Longmore , A J , Vacva , B , Liu , M , Webster , A , Wolscznan , A & Barnes , A 2009 , ' Precision radial velocities in the infrared ' , Astrophysics and Space Science Proceedings , pp. 415-416 .
dc.identifier.otherPURE: 162407
dc.identifier.otherPURE UUID: e0551af6-9bac-4948-b2e6-904a3f9f6a30
dc.identifier.otherdspace: 2299/5942
dc.identifier.otherScopus: 85034653831
dc.description“The original publication is available at” Copyright Springer [Full text of this article is not available in the UHRA]
dc.description.abstractOver 250 extra-solar planets have been discovered to date using a variety of techniques. The majority have been discovered at optical wavelengths from the Doppler shift of F, G and K stars induced by orbiting planets. We have constructed models simulating likely planets around M dwarfs and demonstrated the ability to recover their radial velocity signals in the infrared. We have conducted experiments in the infrared with a brass-board instrument to explore real-world issues. We are thus confident that a stabilised radial velocity spectrometer with a single-shot 1 and 1.7 microns coverage at a resolution of around 70 k can achieve an instrumental radial velocity error of 0.5 m/s. This enables the efficient measurement of radial velocities for M, L and T spectral classes.en
dc.relation.ispartofAstrophysics and Space Science Proceedings
dc.titlePrecision radial velocities in the infrareden
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

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