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dc.contributor.authorCosentino, R.
dc.contributor.authorLovis, C.
dc.contributor.authorPepe, F.
dc.contributor.authorCameron, A.C.
dc.contributor.authorLatham, D.W.
dc.contributor.authorMolinari, E.
dc.contributor.authorUdry, S.
dc.contributor.authorBezawada, N.
dc.contributor.authorBuchschacher, N.
dc.contributor.authorFigueira, P.
dc.contributor.authorFleury, M.
dc.contributor.authorGhedina, A.
dc.contributor.authorGlenday, A.G.
dc.contributor.authorGonzalez, M.
dc.contributor.authorGuerra, J.
dc.contributor.authorHenry, D.
dc.contributor.authorHughes, I.
dc.contributor.authorMaire, C.
dc.contributor.authorMotalebi, F.
dc.contributor.authorPhillips, D.F.
dc.contributor.editorRamsay, Suzanne K.
dc.contributor.editorMcLean, Ian S.
dc.contributor.editorTakami, Hideki
dc.date.accessioned2015-03-03T11:01:04Z
dc.date.available2015-03-03T11:01:04Z
dc.date.issued2014
dc.identifier172271206
dc.identifiera35e1104-9182-43d5-9a22-2b2310a05049
dc.identifier84922676527
dc.identifier000354527800252
dc.identifier.citationCosentino , R , Lovis , C , Pepe , F , Cameron , A C , Latham , D W , Molinari , E , Udry , S , Bezawada , N , Buchschacher , N , Figueira , P , Fleury , M , Ghedina , A , Glenday , A G , Gonzalez , M , Guerra , J , Henry , D , Hughes , I , Maire , C , Motalebi , F & Phillips , D F 2014 , HARPS-N @ TNG, two year harvesting data : performances and results . in S K Ramsay , I S McLean & H Takami (eds) , Ground-based and Airborne Instrumentation for Astronomy V . vol. 9147 , Proceedings of SPIE , vol. 9147 , SPIE , Ground-based and Airborne Instrumentation for Astronomy V , Montréal , United States , 22/06/14 . https://doi.org/10.1117/12.2055813en
dc.identifier.citationconferenceen
dc.identifier.isbn9780819496157
dc.identifier.issn0277-786X
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531326
dc.identifier.urihttps://hdl.handle.net/10023/6155
dc.description.abstractThe planet hunter HARPS-N[1], in operation at the Telescopio Nazionale Galileo (TNG)[13] from April 2012 is a highresolution spectrograph designed to achieve a very high radial velocity precision measurement thanks to an ultra stable environment and in a temperature-controlled vacuum. The main part of the observing time was devoted to Kepler field and achieved a very important result with the discovery of a terrestrial exoplanet. After two year of operation, we are able to show the performances and the results of the instrument.
dc.format.extent2328155
dc.language.isoeng
dc.publisherSPIE
dc.relation.ispartofGround-based and Airborne Instrumentation for Astronomy Ven
dc.relation.ispartofseriesProceedings of SPIEen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleHARPS-N @ TNG, two year harvesting data : performances and resultsen
dc.typeConference itemen
dc.contributor.sponsorEuropean Commissionen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1117/12.2055813
dc.identifier.grantnumberen
dc.identifier.grantnumberST/J001651/1en


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