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An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus

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dc.contributor.authorPhillips, David F.
dc.contributor.authorGlenday, Alex G.
dc.contributor.authorDumusque, Xavier
dc.contributor.authorBuchschacher, Nicolas
dc.contributor.authorCameron, Andrew Collier
dc.contributor.authorCecconi, Massimo
dc.contributor.authorCharbonneau, David
dc.contributor.authorCosentino, Rosario
dc.contributor.authorGhedina, Adriano
dc.contributor.authorHaywood, Raphäelle
dc.contributor.authorLatham, David W.
dc.contributor.authorLi, Chih Hao
dc.contributor.authorLodi, Marcello
dc.contributor.authorLovis, Christophe
dc.contributor.authorMolinari, Emilio
dc.contributor.authorPepe, Francesco
dc.contributor.authorSasselov, Dimitar
dc.contributor.authorSzentgyorgyi, Andrew
dc.contributor.authorUdry, Stephane
dc.contributor.authorWalsworth, Ronald L.
dc.contributor.editorNavarro, Ramón
dc.contributor.editorBurge, James H.
dc.date.accessioned2017-03-15T16:30:16Z
dc.date.available2017-03-15T16:30:16Z
dc.date.issued2016-07-22
dc.identifier.citationPhillips , D F , Glenday , A G , Dumusque , X , Buchschacher , N , Cameron , A C , Cecconi , M , Charbonneau , D , Cosentino , R , Ghedina , A , Haywood , R , Latham , D W , Li , C H , Lodi , M , Lovis , C , Molinari , E , Pepe , F , Sasselov , D , Szentgyorgyi , A , Udry , S & Walsworth , R L 2016 , An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus . in R Navarro & J H Burge (eds) , Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II . , 99126Z , Proceedings of SPIE , vol. 9912 , SPIE , Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II , Edinburgh , United Kingdom , 26/06/16 . https://doi.org/10.1117/12.2232452en
dc.identifier.citationconferenceen
dc.identifier.isbn9781510602038
dc.identifier.issn0277-786X
dc.identifier.otherPURE: 249376721
dc.identifier.otherPURE UUID: 6e4ec453-e066-49a1-9743-3bff6d48834a
dc.identifier.otherScopus: 84996629645
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531522
dc.identifier.otherWOS: 000387747900208
dc.identifier.urihttps://hdl.handle.net/10023/10475
dc.description.abstractWe recently demonstrated sub-m/s sensitivity in measuring the radial velocity (RV) between the Earth and Sun using a simple solar telescope feeding the HARPS-N spectrograph at the Italian National Telescope, which is calibrated with a green astro-comb. We are using the solar telescope to characterize the effects of stellar (solar) RV jitter due to activity on the solar surface with the goal of detecting the solar RV signal from Venus, thereby demonstrating the sensitivity of these instruments to detect true Earth-twin exoplanets.
dc.format.extent8
dc.language.isoeng
dc.publisherSPIE
dc.relation.ispartofAdvances in Optical and Mechanical Technologies for Telescopes and Instrumentation IIen
dc.relation.ispartofseriesProceedings of SPIEen
dc.rights© 2016, SPIE. This work has been made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at proceedings.spiedigitallibrary.org / https://doi.org/10.1117/12.2232452en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectElectronic, Optical and Magnetic Materialsen
dc.subjectCondensed Matter Physicsen
dc.subjectComputer Science Applicationsen
dc.subjectApplied Mathematicsen
dc.subjectElectrical and Electronic Engineeringen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleAn astro-comb calibrated solar telescope to search for the radial velocity signature of Venusen
dc.typeConference itemen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1117/12.2232452


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