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The 3XLSS point source catalogue
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| DOI | 10.1051/0004-6361/201731880 | ||||
| Año | 2018 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
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 deg(2) with a flux limit (at 3 sigma) of similar to 10 15 erg s(-1) cm(-2) in [0.5-2] keV, and similar to 3 x 10(-15) erg s(-1) cm(-2) in [2-10] keV, yielding a 90% completeness limit of 5.8 x 10(-15) and 3.8 x 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 XXL data release.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Chiappetti, L. | - |
Istituto Nazionale di Astrofisica - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia INAF - Italia |
| 2 | Fotopoulou, S. | - |
Univ Geneva - Suiza
Université de Genève - Suiza |
| 3 | Lidman, Chris | Hombre |
Australian Astron Observ - Australia
Australian Astronomical Observatory - Australia |
| 4 | Faccioli, L. | - |
Univ Paris Diderot - Francia
Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia |
| 5 | Pacaud, F. | - |
UNIV BONN - Alemania
Universität Bonn - Alemania |
| 6 | Elyiv, A. | - |
UNIV BOLOGNA - Italia
Ukrainian Acad Sci - Ucrania |
| 7 | Paltani, Stephane | Hombre |
Univ Geneva - Suiza
Université de Genève - Suiza |
| 8 | Pierre, M. | - |
Univ Paris Diderot - Francia
Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia |
| 9 | Plionis, Manolis | Hombre |
Natl Observ Athens - Grecia
Aristotle Univ Thessaloniki - Grecia National Observatory of Athens - Grecia Aristotle University of Thessaloniki - Grecia |
| 10 | Adami, Christophe | Hombre |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| 11 | Alis, S. | - |
Istanbul Univ - Turquía
Istanbul Üniversitesi - Turquía |
| 12 | Altieri, B. | Hombre |
European Space Astron Ctr ESA ESAC - España
European Space Astronomy Centre - España |
| 13 | Baran, Andrzej S. | Hombre |
Liverpool John Moores Univ - Reino Unido
Liverpool John Moores University - Reino Unido |
| 14 | Bolzonella, M. | Mujer |
Istituto Nazionale di Astrofisica - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia INAF - Italia |
| 15 | Bongiorno, A. | Mujer |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Roma - Italia Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 16 | Brown, M. | Hombre |
MONASH UNIV - Australia
Monash University - Australia |
| 17 | Driver, S. | Hombre |
ICRAR - Australia
Univ St Andrews - Reino Unido University of St Andrews - Reino Unido |
| 18 | Elmer, E. | - |
Univ Nottingham - Reino Unido
University of Nottingham - Reino Unido |
| 19 | Franzetti, P. | Hombre |
Istituto Nazionale di Astrofisica - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia INAF - Italia |
| 20 | Grootes, M. | - |
Max Planck Inst Kernphys - Alemania
Max Planck Institute for Nuclear Physics - Alemania Max-Planck-Institut für Kernphysik - Alemania |
| 21 | Guglielmo, V. | - |
Aix Marseille Univ - Francia
Istituto Nazionale di Astrofisica - Italia Laboratoire d'Astrophysique de Marseille - Francia Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 22 | Iovino, A. | - |
Istituto Nazionale di Astrofisica - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia INAF - Italia |
| 23 | Koulouridis, E. | - |
Univ Paris Diderot - Francia
Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia |
| 24 | Lefevre, J. | - |
Univ Paris Diderot - Francia
Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia |
| 25 | Liske, J. | Hombre |
UNIV HAMBURG - Alemania
Universität Hamburg - Alemania |
| 26 | Maurogordato, S. | - |
Univ Nice Sophia Antipolis - Francia
Université Nice Sophia Antipolis - Francia Laboratoire Joseph-Louis Lagrange - Francia |
| 27 | Melnyk, O. | - |
Ukrainian Acad Sci - Ucrania
Univ Zagreb - Croacia Main Astronomical Observatory Nasu - Ucrania University of Zagreb - Croacia |
| 28 | Owers, Matt | Hombre |
Australian Astron Observ - Australia
Macquarie Univ - Australia Australian Astronomical Observatory - Australia Macquarie University - Australia |
| 29 | Poggianti, B. | Mujer |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 30 | Polletta, Mari | Mujer |
Istituto Nazionale di Astrofisica - Italia
Univ Toulouse - Francia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia Université de Toulouse - Francia Université Toulouse III - Paul Sabatier - Francia INAF - Italia |
| 31 | Ségransan, Damien | Hombre |
ESO - Chile
European Southern Observatory Santiago - Chile |
| 32 | Ponman, T. | - |
Univ Birmingham - Reino Unido
University of Birmingham - Reino Unido |
| 33 | Robotham, A. | Hombre |
ICRAR - Australia
Univ St Andrews - Reino Unido University of St Andrews - Reino Unido |
| 34 | Sadibekova, T. | - |
Univ Paris Diderot - Francia
Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia |
| 35 | Steenkamp, R. | Hombre |
Max Planck Inst Kernphys - Alemania
Max Planck Institute for Nuclear Physics - Alemania Max-Planck-Institut für Kernphysik - Alemania |
| 36 | Valtchanov, I. | Hombre |
European Space Astron Ctr ESA ESAC - España
European Space Astronomy Centre - España |
| 37 | Vignali, Cristian | Hombre |
UNIV BOLOGNA - Italia
Istituto Nazionale di Astrofisica - Italia Alma Mater Studiorum Università di Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia INAF - Italia |
| 38 | Wagner, G. | - |
UNIV OXFORD - Reino Unido
Univ Oxford Merton Coll - Reino Unido University of Oxford - Reino Unido Merton College - Reino Unido |
| Fuente |
|---|
| CNRS |
| Science and Technology Facilities Council |
| Australian Astronomical Observatory |
| CNES |
| STFC (UK) |
| Centre National de la Recherche Scientifique |
| California Institute of Technology |
| Ministry of Economy and Technology (BMWi) |
| German Aerospace Agency (DLR) |
| Centre National d'Etudes Spatiales |
| Centre National d’Etudes Spatiales |
| Association pour la recherche sur le cancer |
| Centre National d’Etudes Spatiales |
| Bundesministerium für Wirtschaft und Technologie |
| German Aerospace Agency |
| Bundesministerium fur Wirtschaft und Technologie |
| ESO Very Large Telescope, under the "Large Programme" |
| Appalachian Regional Commission |
| AAO |
| ARC (Australia) |
| TUBITAK-BIDEB through 2219 programme |
| Ministry of Economy and Technology |
| TUBITAK-BIDEB |
| American Academy of Ophthalmology |
| Division of Loan Repayment |
| Agradecimiento |
|---|
| XXL is an international project based around an XMM Very Large Programme surveying two 25 deg<SUP>2</SUP> extragalactic fields at a depth of similar to 5 x 10<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>2</SUP> in [0.5-2] keV. The XXL website is http://irfu.cea.fr/xxl.Multiband information and spectroscopic followup of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/.Based in part on data acquired through the Australian Astronomical Observatory, under programmes A/2016B/107. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France, and of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. The Saclay team acknowledges long-term financial support from the Centre National d'Etudes Spatiales. This paper uses data from the Galaxy And Mass Assembly (GAMA) survey and from the VIMOS Public Extragalactic Redshift Survey (VIPERS). GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/.VIPERS has been performed using the ESO Very Large Telescope, under the "Large Programme" 182. A-0886. The participating institutions and funding agencies are listed at http://vipers.inaf.it.The Saclay group acknowledges long-term support from the Centre National d'Etudes Spatiales (CNES). F. P. acknowledges support by the German Aerospace Agency (DLR) with funds from the Ministry of Economy and Technology (BMWi) through grant 50 OR 1514 and grant 50 OR 1608. S. A. acknowledges a post-doctoral fellowship from TUBITAK-BIDEB through 2219 programme. E. K. thanks CNES and CNRS for support of post-doctoral research. |
| XXL is an international project based around an XMM Very Large Programme surveying two 25 deg2 extragalactic fields at a depth of ∼5 × 10-15 erg s-1 cm-2 in [0.5-2] keV. The XXL website is http://irfu.cea.fr/xxl. Multiband information and spectroscopic followup of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/. Based in part on data acquired through the Australian Astronomical Observatory, under programmes A/2016B/107. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France, and of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. The Saclay team acknowledges long-term financial support from the Centre National d'Etudes Spatiales. This paper uses data from the Galaxy And Mass Assembly (GAMA) survey and from the VIMOS Public Extragalactic Redshift Survey (VIPERS). GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. VIPERS has been performed using the ESO Very Large Telescope, under the "Large Programme" 182.A-0886. The participating institutions and funding agencies are listed at http://vipers.inaf.it. The Saclay group acknowledges long-term support from the Centre National d'Études Spatiales (CNES). F.P. acknowledges support by the German Aerospace Agency (DLR) with funds from the Ministry of Economy and Technology (BMWi) through grant 50 OR 1514 and grant 50 OR 1608. S.A. acknowledges a post-doctoral fellowship from TUBITAK-BIDEB through 2219 programme. E.K. thanks CNES and CNRS for support of post-doctoral research. |
