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dc.contributor.authorBarnes, J.R.
dc.contributor.authorJenkins, J. S.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorRojo, P.
dc.contributor.authorArriagada, P.
dc.contributor.authorJordan, A.
dc.contributor.authorMinniti, D.
dc.contributor.authorTuomi, M.
dc.contributor.authorJeffers, S.V.
dc.contributor.authorPinfield, D.J.
dc.contributor.editorSaglia, R.
dc.date.accessioned2014-07-16T12:30:13Z
dc.date.available2014-07-16T12:30:13Z
dc.date.issued2013
dc.identifier.citationBarnes , J R , Jenkins , J S , Jones , H R A , Rojo , P , Arriagada , P , Jordan , A , Minniti , D , Tuomi , M , Jeffers , S V & Pinfield , D J 2013 , Red Optical Planet Survey : A radial velocity search for low mass M dwarf planets . in R Saglia (ed.) , Hot Planets and Cool Stars . , 05002 , EPJ Web of Conferences , vol. 47 , EDP Sciences , Conference on Hot Planets and Cool Stars , Germany , 12/11/12 . https://doi.org/10.1051/epjconf/20134705002
dc.identifier.citationconference
dc.identifier.issn2100-014X
dc.identifier.otherPURE: 7179676
dc.identifier.otherPURE UUID: b45dfa3d-a3d7-4973-bac1-d46cb296582e
dc.identifier.otherWOS: 000319988900023
dc.identifier.otherScopus: 84877626870
dc.identifier.urihttp://hdl.handle.net/2299/13944
dc.descriptionThis is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
dc.description.abstractWe present radial velocity results from our Red Optical Planet Survey (ROPS), aimed at detecting low-mass planets orbiting mid-late M dwarfs. The similar to 10 ms(-1) precision achieved over 2 consecutive nights with the MIKE spectrograph at Magellan Clay is also found on week long timescales with UVES at VLT. Since we find that UVES is expected to attain photon limited precision of order 2 ms-1 using our novel deconvolution technique, we are limited only by the (en
dc.format.extent4
dc.language.isoeng
dc.publisherEDP Sciences
dc.relation.ispartofHot Planets and Cool Stars
dc.relation.ispartofseriesEPJ Web of Conferences
dc.titleRed Optical Planet Survey : A radial velocity search for low mass M dwarf planetsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionScience & Technology Research Institute
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1051/epjconf/20134705002
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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