J/MNRAS/475/343 2MASS, WISE, and SuperCOSMOS clusters of galaxies (Wen+, 2018)
A catalogue of clusters of galaxies identified from all sky surveys of
2MASS, WISE, and SuperCOSMOS.
Wen Z.L., Han J.L., Yang F.
<Mon. Not. R. Astron. Soc., 475, 343-352 (2018)>
=2018MNRAS.475..343W 2018MNRAS.475..343W (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Redshifts ; Infrared sources ; X-ray sources
Keywords: catalogues - galaxies: clusters: general -
large-scale structure of Universe
Abstract:
We identify 47600 clusters of galaxies from photometric data of Two
Micron All Sky Survey (2MASS), Wide-field Infrared Survey Explorer
(WISE), and SuperCOSMOS, among which 26125 clusters are recognized for
the first time and mostly in the sky outside the Sloan Digital Sky
Survey (SDSS) area. About 90 per cent of massive clusters of
M500>3x1014M☉ in the redshift range of 0.025<z<0.3 have been
detected from such survey data, and the detection rate drops down to
50 per cent for clusters with a mass of M500∼1x1014M☉. Monte
Carlo simulations show that the false detection rate for the whole
cluster sample is less than 5 per cent. By cross-matching with ROSAT
and XMM-Newton sources, we get 779 new X-ray cluster candidates which
have X-ray counterparts within a projected offset of 0.2Mpc.
Description:
By using the photometric redshift data for about 18.4 million galaxies
of 2MASS, WISE, and SuperCOSMOS obtained by Bilicki et al.
(2014ApJS..210....9B 2014ApJS..210....9B) and Bilicki et al. (2016ApJS..225....5B 2016ApJS..225....5B), we
identify 47600 galaxy clusters in the sky survey area of 28000 square
degree. The BCG candidates are first selected by using the criteria of
galaxy magnitude and colour. Clusters are then identified as the
overdensity regions of galaxy counts around the BCG candidates. The
detection rate is as high as 90 per cent for massive clusters of
M500>3x1014M☉ in the redshift range of 0.025<z<0.3, and drops
down to 50 per cent for clusters with a mass of M500∼1x1014M☉.
Among 47600 galaxy clusters, 26125 clusters are identified for the
first time, which are mostly located in the sky outside the SDSS area.
Monte Carlo simulations show that the false detection rate is less
than 5 per cent in general. By cross-matching with ROSAT and
XMM-Newton sources, we find 779 new X-ray cluster candidates.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 93 21475 21475 known clusters of galaxies recognized from
the survey data of SuperCOSMOS, WISE, and 2MASS
table2.dat 75 26125 26125 newly identified clusters of galaxies from
the survey data of SuperCOSMOS, WISE, and 2MASS
table3.dat 106 1490 779 new X-ray cluster candidates and 711 known
X-ray clusters from cross-matching with ROSAT
and XMM-Newton sources
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See also:
II/311 : WISE All-Sky Data Release (Cutri+ 2012)
II/328 : AllWISE Data Release (Cutri+ 2013)
II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)
IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)
IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)
IX/30 : Second ROSAT PSPC Catalog (ROSAT, 2000)
IX/59 : XMM-Newton Serendipitous Source Catalogue 4XMM-DR9 (Webb+, 2020)
J/A+A/588/A103 : Second ROSAT all-sky survey (2RXS) source catalog
(Boller+, 2016)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 16 A16 --- Name Name (JHHMMSS.s+DDMMSS)
19- 27 F9.5 deg RAdeg Cluster BCG right ascension (J2000)
30- 38 F9.5 deg DEdeg Cluster BCG declination (J2000)
41- 46 F6.4 --- z Cluster redshift
50 I1 --- f_z [0/1] photometric (0) or spectroscopic (1)
redshift
53- 57 F5.2 mag RBCG Cluster BCG R magnitude
60- 64 F5.2 --- S/N S/N of the overdensity for cluster recognition
66- 71 F6.2 --- RL* Cluster richness
74- 93 A20 --- OCat Other catalogues containing the cluster (1)
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Note (1): Other catalogues containing the cluster as follows:
Abell = Abell 1958ApJS....3..211A 1958ApJS....3..211A, Cat. VII/4;
Abell et al. 1989ApJS...70....1A 1989ApJS...70....1A, Cat. VII/110)
Zwicky = Zwicky et al., 1961, Cat. VII/49/)
BM78 = Braid & MacGillivray, 1978MNRAS.182..241B 1978MNRAS.182..241B)
GHO = Gunn, Hoessel & Oke, 1986, Cat. J/ApJ/306/30)
EDCC = Lumsden et al., 1992MNRAS.258....1L 1992MNRAS.258....1L, Cat. VII/175)
APM = Dalton et al., 1997, Cat. J/MNRAS/289/263)
CE = Goto et al., 2002, Cat. J/AJ/123/1807)
NSCS = Lopes et al., 2004, Cat. J/AJ/128/1017)
C4 = Miller et al., 2005, Cat. J/AJ/130/968)
TES+06 = Tago et al., 2006, Cat. J/AN/327/365)
maxBCG = Koester et al., 2007, Cat. J/ApJ/660/239)
YMV+07 = Yang et al., 2007ApJ...671..153Y 2007ApJ...671..153Y)
NSC = Gal et al., 2009, Cat. J/AJ/137/2981)
GMBCG = Hao et al., 2010, Cat. J/ApJS/191/254)
AMF = Szabo et al., 2011, Cat. J/ApJ/736/21;
Banerjee et al., 2018, Cat. J/other/NewA/58.61)
MCXC = Piffaretti et al., 2011, Cat. J/A+A/534/A109)
GMB+11 = Geach, Murphy & Bower, 2011, Cat. J/MNRAS/413/3059)
WH11 = Wen & Han, 2011, Cat. J/ApJ/734/68)
WHL = Wen et al., 2012, Cat. J/ApJS/199/34;
Wen & Han, 2015, Cat. J/ApJ/807/178)
MSPM = Smith et al., 2012, Cat. J/MNRAS/422/25)
TTL12 = Tempel, Tago & Liivamagi, 2012, Cat. J/A+A/540/A106)
RXSC = Chon, Bohringer & Nowak, 2013, Cat. J/MNRAS/429/3272)
redMaPPer = Rykoff et al., 2014, Cat. J/ApJ/785/104, 2016, Cat. J/ApJS/224/1)
CAMIRA = Oguri 2014, Cat. J/MNRAS/444/147)
SPT = Bleem et al. 2015, Cat. J/ApJS/216/27)
SWXCS = Liu et al. 2015, Cat. J/ApJS/216/28)
DAB+15 = Durret et al. 2015, Cat. J/A+A/578/A79)
LCS = Bleem et al. 2015, Cat. J/ApJS/216/20)
PSZ2 = Planck Collaboration XXVII 2016, Cat. J/A+A/594/A27)
TKT16 = Tempel et al. 2016, Cat. J/A+A/588/A14)
XLSSC = Pacaud et al. 2016A&A...592A...2P 2016A&A...592A...2P, Cat. IX/49)
KDR2 = Radovich et al. 2017, Cat. J/A+A/598/A107)
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 20 A20 --- Name WHY name (JHHMMSS.s+DDMMSS)
23- 31 F9.5 deg RAdeg Cluster BCG right ascension (J2000)
34- 42 F9.5 deg DEdeg Cluster BCG declination (J2000)
45- 50 F6.4 --- z Cluster redshift
54 I1 --- f_z [0/1] photometric (0) or spectroscopic (1)
redshift
57- 61 F5.2 mag RBCG Cluster BCG R magnitude
64- 68 F5.2 --- S/N S/N of the overdensity for cluster recognition
70- 75 F6.2 --- RL* Cluster richness
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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2- 4 A3 --- WHY [WHY] WHY for known clusters in previous
optical, SZ or X-ray cluster catalogues
(see Table 1)
6- 21 A16 --- Name Cluster name, JHHMMSS.s+DDMMSS
24- 32 F9.5 deg RAdeg Cluster right ascension (J2000)
35- 43 F9.5 deg DEdeg Cluster declination (J2000)
46- 51 F6.4 --- z Cluster redshift
53- 73 A21 --- XName Name of X-ray source with J2000 coordinates
75- 80 F6.3 10-15W/m2 FX X-ray flux in 0.1-2.4keV band for ROSAT
sources and in 2.0-4.5keV for XMM-Newton
sources (in 10-12erg/cm2/s)
83- 87 F5.3 10-15W/m2 e_FX rms uncertainty on FX
90- 94 F5.3 Mpc rp Projected offset between the X-ray source
and the cluster
97-106 A10 --- OCat Previous X-ray cluster catalogue (1)
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Note (1): Previous X-ray cluster catalogue as follows:
MCXC = Piffaretti et al., 2011, Cat. J/A+A/534/A109),
2XMMi-SDSS = Takey et al., 2011, Cat. J/A+A/534/A120; Takey, Schwope & Lamer,
2013, Cat. J/A+A/558/A75, 2014, Cat. J/A+A/564/A54),
WYS+14 = Wang et al. 2014, Cat. J/MNRAS/439/611),
WHL09 = Wen et al. 2009, Cat. J/ApJS/183/197),
SWXCS = Liu et al. 2015, Cat. J/ApJS/216/28),
XLSSC = Pacaud et al. 2016A&A...592A...2P 2016A&A...592A...2P, Cat. IX/49)
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History:
From electronic version of the journal
(End) Patricia Vannier [CDS] 24-Mar-2021