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Table 3

List of VTA-detected cluster/group candidates.

ID RA Dec σ phot k T 300 kpc r 500 M 500,MT
[h m s] [d m s] [× 1042 erg s-1] [keV] [kpc] [× 1013 M⊙ ]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
XLSSC 081 02 12 12* –06 12 39* 0.42 0.04 0.428* 14.9* 1.7* 549* 7*
XLSSC 082 02 10 51* –06 10 44* 0.42 0.04 0.424* 17.1* 3.9* 878* 29*
XLSSC 083 02 10 56* –06 11 54* 0.42 0.03 0.430* 31.3* 4.8* 990* 41*
XLSSC 084 02 11 03* –06 12 47* 0.42 0.04 0.430* 13.8* 4.5* 955* 37*
XLSSC 085 02 11 29* –06 11 47* 0.43 0.03 0.428* 28.3* 4.8* 985* 41*
XLSSC 086 02 11 14* –06 09 44* 0.41 0.04 0.424* 11.2* 2.6* 698* 15*
XLSSC 099 02 12 53 –06 12 07 0.43 0.04 0.3911 14.4 5.1 1038 47
VTA01 02 11 10 –06 13 22 0.40 0.04 ... <7.3 <1.8 <560.6 <7.7
VTA02 02 10 58 –06 13 53 0.39 0.05 ... <9.3 <1.9 <590.2 <9.0
VTA03 02 11 01 –06 15 50 0.43 0.04 ... <5.9 <1.6 <535.2 <6.7
VTA04 02 12 18 –06 10 30 0.41 0.03 ... <9.1 <1.9 <586.9 <8.8
VTA05 02 12 20 –06 12 01 0.42 0.05 ... <9.9 <2.0 <597.1 <9.3
VTA06 02 12 30 –06 12 13 0.43 0.03 ... <11.7 <2.1 <618.9 <10.3
VTA07 02 11 50 –06 13 28 0.43 0.03 ... <7.5 <1.8 <563.3 <7.8
VTA08 02 12 01 –06 09 36 0.43 0.04 ... <8.83 <2.04 <606.6 <9.7
VTA09 02 13 06 –06 14 13 0.47 0.06 ... <8.8 <1.9 <582.7 <8.6
VTA10 02 13 01 –06 08 24 0.39 0.06 ... <11.9 <2.30 <649.7 <11.9

Notes. For clusters detected in the X-rays the X-ray ID (XLSSC) is adopted. Cluster candidates with unavailable spectroscopic redshift are marked by ellipses (...). Central right ascension and declination of regions shown in Figs. 7, 11 and 12 are given in Cols. (2) and (3). For the galaxies satisfying the VTA overdensity threshold and potentially belonging to the given structure as suggested by the circular or elliptical areas in Figs. 7, 11 and 12, the mean photometric redshift and its standard deviation are given in Cols. (4) and (5), respectively. The spectroscopic redshift is given in Col. (6) (where available). Where available, X-ray luminosity in units of erg s-1, temperature in keV, r500 in kpc and M500,MT in units of solar mass (M⊙) are given in Cols. (7)−(10), respectively (as described in Paper VII; Paper III). M500,MT for XLSSC clusters has been derived in Paper IV using MWL − T relation. For X-ray non-detected VTA structures, 3σ upper limits are given (see Sect. 4 for details).

(*)

Taken from Paper VII.

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