The XXL Survey : XXVII. The 3XLSS point source catalogue
Date
12/2018Author
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Abstract
We 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.
Citation
Chiappetti , 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/10.1051/0004-6361/201731880
Publication
Astronomy & Astrophysics
Status
Peer reviewed
ISSN
0004-6361Type
Journal article
Rights
Copyright © 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/10.1051/0004-6361/201731880
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