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dc.contributor.authorChiappetti, L.
dc.contributor.authorFotopoulou, S.
dc.contributor.authorLidman, C.
dc.contributor.authorFaccioli, L.
dc.contributor.authorPacaud, F.
dc.contributor.authorElyiv, A.
dc.contributor.authorPaltani, S.
dc.contributor.authorPierre, M.
dc.contributor.authorPlionis, M.
dc.contributor.authorAdami, C.
dc.contributor.authorAlis, S.
dc.contributor.authorAltieri, B.
dc.contributor.authorBaldry, I.
dc.contributor.authorBolzonella, M.
dc.contributor.authorBongiorno, A.
dc.contributor.authorBrown, M.
dc.contributor.authorDriver, S.
dc.contributor.authorElmer, E.
dc.contributor.authorFranzetti, P.
dc.contributor.authorGrootes, M.
dc.contributor.authorGuglielmo, V.
dc.contributor.authorIovino, A.
dc.contributor.authorKoulouridis, E.
dc.contributor.authorLefevre, J. P.
dc.contributor.authorLiske, J.
dc.contributor.authorMaurogordato, S.
dc.contributor.authorMelnyk, O.
dc.contributor.authorOwers, M.
dc.contributor.authorPoggianti, B.
dc.contributor.authorPolletta, M.
dc.contributor.authorPompei, E.
dc.contributor.authorPonman, T.
dc.contributor.authorRobotham, A.
dc.contributor.authorSadibekova, T.
dc.contributor.authorTuffs, R.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVignali, C.
dc.contributor.authorWagner, G.
dc.date.accessioned2019-10-16T10:30:05Z
dc.date.available2019-10-16T10:30:05Z
dc.date.issued2018-12
dc.identifier.citationChiappetti , L , Fotopoulou , S , Lidman , C , Faccioli , L , Pacaud , F , Elyiv , A , Paltani , S , Pierre , M , Plionis , M , Adami , C , Alis , S , Altieri , B , Baldry , I , Bolzonella , M , Bongiorno , A , Brown , M , Driver , S , Elmer , E , Franzetti , P , Grootes , M , Guglielmo , V , Iovino , A , Koulouridis , E , Lefevre , J P , Liske , J , Maurogordato , S , Melnyk , O , Owers , M , Poggianti , B , Polletta , M , Pompei , E , Ponman , T , Robotham , A , Sadibekova , T , Tuffs , R , Valtchanov , I , Vignali , C & Wagner , G 2018 , ' The XXL Survey : XXVII. The 3XLSS point source catalogue ' , Astronomy & Astrophysics , vol. 620 , A12 , pp. 1-18 . https://doi.org/10.1051/0004-6361/201731880en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 261905980
dc.identifier.otherPURE UUID: 9c8fe230-5653-476b-a45a-1fef4afd4a1b
dc.identifier.otherArXiv: http://arxiv.org/abs/1810.03929v1
dc.identifier.otherScopus: 85057242111
dc.identifier.otherWOS: 000450930100012
dc.identifier.urihttps://hdl.handle.net/10023/18687
dc.description.abstractWe present the version of the point source catalogue of the XXL Survey that was used, in part, in the first series of XXL papers. In this paper we release, in our database in Milan and at CDS: (i) the X-ray source catalogue with 26 056 objects in two areas of 25 deg2 with a flux limit (at 3σ) of ~10−15 erg s−1 cm−2 in [0.5–2] keV, and ~ 3 × 10−15 erg s−1 cm−2 in [2–10] keV, yielding a 90% completeness limit of 5.8 × 10−15 and 3.8 × 10−14 respectively; (ii) the associated multiwavelength catalogues with candidate counterparts of the X-ray sources in the infrared, near-infrared, optical, and ultraviolet (plus spectroscopic redshift when available); and (iii) a catalogue of spectroscopic redshifts recently obtained in the southern XXL area. We also present the basic properties of the X-ray point sources and their counterparts. Other catalogues described in the second series of XXL papers will be released contextually, and will constitute the second XXLdata release.
dc.format.extent18
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rightsCopyright © 2018 ESO. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at https://doi.org/10.1051/0004-6361/201731880en
dc.subjectSurveysen
dc.subjectX-rays : generalen
dc.subjectCatalogsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe XXL Survey : XXVII. The 3XLSS point source catalogueen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201731880
dc.description.statusPeer revieweden


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