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The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters - XVII. Public Catalogue Release

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dc.contributor.authorNardiello, D.en
dc.contributor.authorLibralato, M.en
dc.contributor.authorPiotto, G.en
dc.contributor.authorAnderson, J.en
dc.contributor.authorBellini, A.en
dc.contributor.authorAparicio, A.en
dc.contributor.authorBedin, L. R.en
dc.contributor.authorCassisi, S.en
dc.contributor.authorGranata, V.en
dc.contributor.authorKing, I. R.en
dc.contributor.authorLucertini, F.en
dc.contributor.authorMarino, A. F.en
dc.contributor.authorMilone, A. P.en
dc.contributor.authorOrtolani, S.en
dc.contributor.authorPlatais, I.en
dc.contributor.authorvan der Marel, R. P.en
dc.date.accessioned2025-03-16T11:30:29Z
dc.date.available2025-03-16T11:30:29Z
dc.date.issued2018-12-11en
dc.description.abstractIn this paper, we present the astrophotometric catalogues of 56 globular clusters and one open cluster. Astrometry and photometry are mainly based on images collected within the 'HST Legacy Survey of Galactic Globular Clusters: Shedding UV Light on Their Populations and Formation' (GO-13297, PI: Piotto), and the 'ACS Survey of Galactic Globular Clusters' (GO-10775, PI: Sarajedini). For each source in the catalogues for which we have reliable proper motion, we also publish a membership probability for separation of field and cluster stars. These new catalogues, which we make public in Mikulski Archive for Space Telescopes, replace previous catalogues by Paper VIII of this series.en
dc.description.sponsorshipThis work has made use of data from the European Space Agency (ESA) mission Gaia (http://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, http: //www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. DN and GP acknowledge partial support by the Università degli Studi di Padova Progetto di Ateneo CPDA141214 and BIRD178590 and by INAF under the program PRIN-INAF2014. ML and AB acknowledge support from STScI grant GO 13297. AA, SC, and GP acknowledge partial support by the Spanish Ministry of Economy and Competitiveness and the Spanish Ministry of Science, Innovation and Universities (grants AYA2013-42781-P and AYA2017-89841-P). AA acknowledges partial support by the Instituto de Astrofìsica de Canarias (grant 310394). APM acknowledges support by the European Research Council through the ERC-StG 2016 project 716082 ’GALFOR’. AFM has been supported by the Australian Research Council through Discovery Early Career Researcher Award DE160100851.Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555.All of the data products are available at MAST as a High Level Science Product under the project HUGS: https://archive.stsci.edu/prepds/hugs/en
dc.description.statustrueen
dc.format.extent12en
dc.identifier.otherresearchoutputwizard:u3102795xPUB37en
dc.identifier.otherScopus:85054218726en
dc.identifier.otherWOS:WOS:000450984100042en
dc.identifier.urihttps://dspace-test.anu.edu.au/handle/1885/733718483
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85054218726&partnerID=8YFLogxKen
dc.language.isoEnglishen
dc.rightsPublisher Copyright: © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.en
dc.sourceMonthly Notices of the Royal Astronomical Societyen
dc.subjectCatalogues -Hertzsprung-Russell and colour- magnitude diagramsen
dc.subjectGlobular clusters: generalen
dc.subjectStars: Population IIen
dc.subjectTechniques: photometricen
dc.titleThe Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters - XVII. Public Catalogue Releaseen
dc.typeArticleen
local.bibliographicCitation.lastpage3393en
local.bibliographicCitation.startpage3382en
local.contributor.affiliationNardiello, D.; University of Paduaen
local.contributor.affiliationLibralato, M.; Space Telescope Science Instituteen
local.contributor.affiliationPiotto, G.; University of Paduaen
local.contributor.affiliationAnderson, J.; Space Telescope Science Instituteen
local.contributor.affiliationBellini, A.; Space Telescope Science Instituteen
local.contributor.affiliationAparicio, A.; Instituto de Astrofísica de Canariasen
local.contributor.affiliationBedin, L. R.; Astronomical Observatory of Paduaen
local.contributor.affiliationCassisi, S.; Istituto Nazionale di Astrofsica - Osservatorio Astronomico d’Abruzzoen
local.contributor.affiliationGranata, V.; University of Paduaen
local.contributor.affiliationKing, I. R.; University of Washingtonen
local.contributor.affiliationLucertini, F.; University of Paduaen
local.contributor.affiliationMarino, A. F.; RSAA - Stromlo, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationMilone, A. P.; University of Paduaen
local.contributor.affiliationOrtolani, S.; University of Paduaen
local.contributor.affiliationPlatais, I.; Johns Hopkins Universityen
local.contributor.affiliationvan der Marel, R. P.; Space Telescope Science Instituteen
local.identifier.citationvolume481en
local.identifier.doi10.1093/mnras/sty2515en
local.identifier.purec894c24c-65b7-424d-be4d-ae91eac4c115en
local.type.statusPublisheden

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