Dataciencia

Colección SciELO Chile

SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release

Indexado

WoS	WOS:000577137200104
Scopus	SCOPUS_ID:85096896064

DOI

10.1093/MNRAS/STAA2066

Año

2020

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

SPIDERS (The SPectroscopic IDentification of eROSITA Sources) is a large spectroscopic programme for X-ray selected galaxy clusters as part of the Sloan Digital Sky Survey-IV (SDSS-IV). We describe the final data set in the context of SDSS Data Release 16 (DR16): the survey overall characteristics, final targeting strategies, achieved completeness, and spectral quality, with special emphasis on its use as a galaxy cluster sample for cosmology applications. SPIDERS now consists of about 27 000 new optical spectra of galaxies selected within 4000 photometric red sequences, each associated with an X-ray source. The excellent spectrograph efficiency and a robust analysis pipeline yield a spectroscopic redshift measurement success rate exceeding 98 per cent, with a median velocity accuracy of 20 kms(-1) (at z = 0.2). Using the catalogue of 2740 X-ray galaxy clusters confirmed with DR16 spectroscopy, we reveal the 3D map of the galaxy cluster distribution in the observable Universe up to z similar to 0.6. We highlight the homogeneity of the member galaxy spectra among distinct regions of the galaxy cluster phase space. Aided by accurate spectroscopic redshifts and by a model of the sample selection effects, we compute the galaxy cluster X-ray luminosity function and we present its lack of evolution up to z = 0.6. Finally we discuss the prospects of forthcoming large multiplexed spectroscopic programmes dedicated to follow up the next generation of all-sky X-ray source catalogues.

Revista

Revista	ISSN
Monthly Notices Of The Royal Astronomical Society	0035-8711

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Clerc, Nicolas	Hombre	Univ Toulouse - Francia Universite Paul Sabatier Toulouse III - Francia Université Toulouse III - Paul Sabatier - Francia Institut de Recherche en Astrophysique et Planétologie (IRAP) - Francia
2	Kirkpatrick, C. C.	Hombre	Univ Helsinki - Finlandia Helsinki Inst Phys - Finlandia Helsingin Yliopisto - Finlandia Helsinki Institute of Physics - Finlandia
3	Finoguenov, A.	Hombre	Univ Helsinki - Finlandia Max Planck Inst Extraterr Phys - Alemania Helsingin Yliopisto - Finlandia Max Planck Institute for Extraterrestrial Physics - Alemania
4	Capasso, R.	Mujer	Stockholm Univ - Suecia Stockholms universitet - Suecia
5	Cora, Sofia A.	Mujer	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
6	Damsted, S.	Mujer	Univ Helsinki - Finlandia Helsingin Yliopisto - Finlandia
7	Furnell, K.	-	Liverpool John Moores Univ - Reino Unido Liverpool John Moores University - Reino Unido
8	Kukkola, A. E.	-	Univ Helsinki - Finlandia Helsingin Yliopisto - Finlandia
9	Ider Chitham, J.	-	Max Planck Institute for Extraterrestrial Physics - Alemania Max Planck Inst Extraterr Phys - Alemania
9	Chitham, Jacob Ider	Hombre	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
10	Merloni, A.	Mujer	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
11	Pannella, M.	Hombre	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
12	Gueguen, A.	Hombre	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
13	Dwelly, Tom	-	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
14	COLLINS, CHRISTOPHER ALFRED	Hombre	Liverpool John Moores Univ - Reino Unido Liverpool John Moores University - Reino Unido
15	Saro, A.	Hombre	UNIV TRIESTE - Italia IFPU Inst Fundamental Phys Universe - Italia Istituto Nazionale di Astrofisica - Italia Università degli Studi di Trieste - Italia Institute for Fundamental Physics of the Universe - Italia Osservatorio Astronomico di Trieste - Italia IFPU - Institute for Fundamental Physics of the Universe - Italia INAF Osservatorio Astron Trieste - Italia
16	Erfanianfar, G.	-	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
17	Schneider, D. P.	Hombre	PENN STATE UNIV - Estados Unidos Pennsylvania State University - Estados Unidos
18	Brownstein, Joel	Hombre	Univ Utah - Estados Unidos The University of Utah - Estados Unidos
19	Mamon, Gary A.	Hombre	Inst Astrophys Paris - Francia Sorbonne Univ - Francia Sorbonne Université - Francia
20	Padilla, Nelson D.	Hombre	Pontificia Universidad Católica de Chile - Chile
21	Jullo, Eric	Hombre	Aix Marseille Univ - Francia Laboratoire d'Astrophysique de Marseille - Francia Aix Marseille Université - Francia
22	Bizyaev, Dmitry	Hombre	Apache Point Observ - Estados Unidos Apache Point Observatory - Estados Unidos

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Origen de Citas Identificadas

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 16.67 %
Citas No-identificadas: 83.33 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 16.67 %
Citas No-identificadas: 83.33 %

Financiamiento

Fuente
National Science Foundation
Universidad Nacional Autónoma de México
U.S. Department of Energy
Ohio State University
Vanderbilt University
NASA
Yale University
National Aeronautics and Space Administration
Max Planck Society
Alfred P. Sloan Foundation
U.S. Department of Energy Office of Science
University of Arizona
Brazilian Participation Group
Carnegie Mellon University
French Participation Group
Instituto de Astrofisica de Canarias
Johns Hopkins University
Lawrence Berkeley National Laboratory
New York University
Pennsylvania State University
University of Portsmouth
University of Utah
University of Virginia
University of Washington
CNES
Carnegie Institution for Science
Chilean Participation Group
Harvard-Smithsonian Center for Astrophysics
Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
Korean Participation Group
Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
Max-Planck-Institut fur Astrophysik (MPA Garching)
Max-Planck-Institut fur Extraterrestrische Physik (MPE)
National Astronomical Observatories of China
University of Notre Dame
Observatario Nacional/MCTI
Shanghai Astronomical Observatory
United Kingdom Participation Group
University of Colorado Boulder
University of Oxford
University of Wisconsin
Higher Education Funding Council for England
DFG cluster of excellence 'Origin and Structure of the Universe'
ESA Member States
Horizon 2020 Framework Programme
Japanese Monbukagakusho
NewMexico State University
Center for HighPerformance Computing at the University of Utah
Leibniz Institut f ur Astrophysik Potsdam (AIP)
FAREMIUR grant 'ClustersXEuclid'
ERCStG 'ClustersXCosmo'

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
The authors thank the referee for their comments which increased the quality of this paper. The authors thank E. Rykoff for providing the data of Fig. 5. Some of the results in this paper have been derived using the HEALPIX (Gorski et al. 2005) package, the MATPLOTLIB package (Hunter 2007), and ASTROPY,7 (Astropy Collaboration 2013; Price-Whelan et al. 2018). This research has made use of 'Aladin sky atlas' developed at CDS, Strasbourg Observatory, France (Bonnarel et al. 2000; Boch & Fernique 2014). It has made use of TOPCAT (Taylor 2005). Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This work was supported by CNES. AF, CK, and JIC acknowledge travel support from the Finnish Centre for Astronomy with ESO (FINCA). NC acknowledges travel support from the Institut Francais de Finlande, the Embassy of France in Finland, the French Ministry of Higher Education, Research and Innovation, the Finnish Society of Sciences and Letters and the Finnish Academy of Science and Letters. CK and NC acknowledge this research was supported by the DFG cluster of excellence 'Origin and Structure of the Universe' (www.universe-cluster.de).AS is supported by the ERCStG 'ClustersXCosmo' grant agreement 716762, and by the FAREMIUR grant 'ClustersXEuclid' R165SBKTMA. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSSIV acknowledges support and resources from the Center for HighPerformance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut f ur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, NewMexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England.

Agradecimiento

The authors thank the referee for their comments which increased the quality of this paper. The authors thank E. Rykoff for providing the data of Fig. 5. Some of the results in this paper have been derived using the HEALPIX (Gorski et al. 2005) package, the MATPLOTLIB package (Hunter 2007), and ASTROPY,7 (Astropy Collaboration 2013; Price-Whelan et al. 2018). This research has made use of 'Aladin sky atlas' developed at CDS, Strasbourg Observatory, France (Bonnarel et al. 2000; Boch & Fernique 2014). It has made use of TOPCAT (Taylor 2005). Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This work was supported by CNES. AF, CK, and JIC acknowledge travel support from the Finnish Centre for Astronomy with ESO (FINCA). NC acknowledges travel support from the Institut Francais de Finlande, the Embassy of France in Finland, the French Ministry of Higher Education, Research and Innovation, the Finnish Society of Sciences and Letters and the Finnish Academy of Science and Letters. CK and NC acknowledge this research was supported by the DFG cluster of excellence 'Origin and Structure of the Universe' (www.universe-cluster.de).AS is supported by the ERCStG 'ClustersXCosmo' grant agreement 716762, and by the FAREMIUR grant 'ClustersXEuclid' R165SBKTMA. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSSIV acknowledges support and resources from the Center for HighPerformance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut f ur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, NewMexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England.

Muestra la fuente de financiamiento declarada en la publicación.

Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección