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dc.contributor.authorPancino, E.
dc.contributor.authorAltavilla, G.
dc.contributor.authorMarinoni, S.
dc.contributor.authorCocozza, G.
dc.contributor.authorCarrasco, J. M.
dc.contributor.authorBellazzini, M.
dc.contributor.authorBragaglia, A.
dc.contributor.authorFederici, L.
dc.contributor.authorRossetti, E.
dc.contributor.authorCacciari, C.
dc.contributor.authorNunez, L. Balaguer
dc.contributor.authorCastro, A.
dc.contributor.authorFigueras, F.
dc.contributor.authorPecci, F. Fusi
dc.contributor.authorGalleti, S.
dc.contributor.authorGebran, M.
dc.contributor.authorJordi, C.
dc.contributor.authorLardo, C.
dc.contributor.authorMasana, E.
dc.contributor.authorMonguio Montells, Maria
dc.contributor.authorMontegriffo, P.
dc.contributor.authorRagaini, S.
dc.contributor.authorSchuster, W.
dc.contributor.authorTrager, S.
dc.contributor.authorVilardell, F.
dc.contributor.authorVoss, H.
dc.date.accessioned2017-04-25T15:05:29Z
dc.date.available2017-04-25T15:05:29Z
dc.date.issued2012-11-01
dc.identifier.citationPancino , E , Altavilla , G , Marinoni , S , Cocozza , G , Carrasco , J M , Bellazzini , M , Bragaglia , A , Federici , L , Rossetti , E , Cacciari , C , Nunez , L B , Castro , A , Figueras , F , Pecci , F F , Galleti , S , Gebran , M , Jordi , C , Lardo , C , Masana , E , Monguio Montells , M , Montegriffo , P , Ragaini , S , Schuster , W , Trager , S , Vilardell , F & Voss , H 2012 , ' The Gaia spectrophotometric standard stars survey. I. Preliminary results ' , Monthly Notices of the Royal Astronomical Society , vol. 426 , no. 3 , pp. 1767-1781 . https://doi.org/10.1111/j.1365-2966.2012.21766.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 11126261
dc.identifier.otherPURE UUID: 43cd4634-3b32-42bc-86f3-1133f82ee7dd
dc.identifier.otherArXiv: http://arxiv.org/abs/1207.6042v1
dc.identifier.otherScopus: 84867618688
dc.identifier.urihttp://hdl.handle.net/2299/18011
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2012 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. The version of record is available online at doi:10.1111/j.1365-2966.2012.21766.x
dc.description.abstractWe describe two ground based observing campaigns aimed at building a grid of approximately 200 spectrophotometric standard stars (SPSS), with an internal ~1% precision and tied to Vega within ~3%, for the absolute flux calibration of data gathered by Gaia, the ESA astrometric mission. The criteria for the selection and a list of candidates are presented, together with a description of the survey strategy and the adopted data analysis methods. We also discuss a short list of notable rejected SPSS candidates and difficult cases, based on identification problems, literature discordant data, visual companions, and variability. In fact, all candidates are also monitored for constancy (within \pm5 mmag, approximately). In particular, we report on a CALSPEC standard, 1740346, that we found to be a delta Scuti variable during our short-term monitoring (1-2 h) campaign.en
dc.format.extent15
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectTechniques: photometric
dc.subjecttechniques: spectroscopic
dc.subjectcatalogues
dc.subjectstars: variables: : δ Scuti.
dc.titleThe Gaia spectrophotometric standard stars survey. I. Preliminary resultsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2012-07-20
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2012.21766.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeopenAccess


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