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HARPS-N @ TNG, two year harvesting data : performances and results

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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.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.otherPURE: 172271206
dc.identifier.otherPURE UUID: a35e1104-9182-43d5-9a22-2b2310a05049
dc.identifier.otherScopus: 84922676527
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531326
dc.identifier.otherWOS: 000354527800252
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.language.isoeng
dc.publisherSPIE
dc.relation.ispartofGround-based and Airborne Instrumentation for Astronomy Ven
dc.relation.ispartofseriesProceedings of SPIEen
dc.rightsRosario Cosentino, Christophe Lovis, Francesco Pepe, Andrew C. Cameron, et al., "HARPS-N @ TNG, two year harvesting data: performances and results," Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 9147, 2014. Copyright 2014 Society of Photo Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.en
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.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1117/12.2055813
dc.identifier.grantnumberen
dc.identifier.grantnumberST/J001651/1en


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