Open Access

Table D.1.

Sub-selection of the eRASS1 cluster catalogue following the constraints described in Sect. 2.1.

CLUSTER ID RA(a) DEC RAOPT(b) DECOPT BEST_Z(c) EXT_LIKE(d) PCONT(e)
[°] [°] [°] [°]
CAHA/Omega2000

1eRASS J025044.2−044309 42.68 −4.72 42.69 −4.72 1.02 ± 0.02 7.35 0.00
1eRASS J031350.5−000546 48.46 −0.10 48.44 −0.09 1.15 ± 0.02 5.06 0.10
1eRASS J033041.6−053608 52.67 −5.60 52.67 −5.60 1.00 ± 0.02 5.99 0.31
1eRASS J042710.8−155324 66.80 −15.89 66.81 −15.89 1.18 ± 0.03 5.85 0.01
1eRASS J043901.1−022852 69.75 −2.48 69.75 −2.48 1.07 ± 0.03 5.25 0.60
1eRASS J053425.5−183444 83.61 −18.58 83.60 −18.59 1.00 ± 0.03 6.91 0.92
1eRASS J085742.5−054517 134.43 −5.75 134.44 −5.75 1.17 ± 0.02 7.00 0.00
1eRASS J091715.4−102343 139.31 −10.40 139.32 −10.40 0.96 ± 0.02 5.77 0.06
1eRASS J094854.3+133740 147.23 13.63 147.23 13.63 1.08 ± 0.03 9.33 0.01
1eRASS J102148.4+225133 155.45 22.86 155.46 22.86 1.12 ± 0.03 5.99 0.00
1eRASS J113751.5+072839 174.46 7.48 174.46 7.47 0.94 ± 0.02 7.74 0.04
1eRASS J124634.6+252236 191.64 25.38 191.64 25.38 1.07 ± 0.02 5.32 0.00
1eRASS J133333.8+062920 203.39 6.49 203.38 6.48 1.14 ± 0.02 6.57 0.00
1eRASS J133801.7+175957 204.51 18.00 204.51 17.99 1.21 ± 0.03 5.29 0.00
1eRASS J140945.2−130101 212.44 −13.02 212.42 −13.02 0.99 ± 0.02 6.49 0.00
1eRASS J142000.6+095651 215.00 9.95 215.01 9.94 1.19 ± 0.02 5.74 0.00
1eRASS J145552.2−030618 223.97 −3.11 223.96 −3.09 1.19 ± 0.05 8.44 0.00

WST/3KK

1eRASS J051425.6−093653 78.61 -9.61 78.61 -9.62 0.72 ± 0.02 15.47 0.00
1eRASS J115512.7+125759 178.80 12.97 178.80 12.97 1.02 ± 0.02 3.24 0.00
1eRASS J121051.6+315520 182.72 31.92 182.73 31.91 0.97 ± 0.01 3.92 0.00
1eRASS J140945.2−130101 212.44 -13.02 212.42 -13.02 0.99 ± 0.02 6.49 0.00

Notes.

a

X-Ray centre of the respective cluster.

b

Optical cluster centre found by Kluge et al. (2024).

c

"Best" redshift estimate assigned to the cluster in Kluge et al. (2024) (see text).

d

Likelihood difference of the source to be extended compared to being a point source (see Sect. 2.1 and Brunner et al. 2022).

e

Estimate of the detection to be a contaminant due to noise, projection effects and point sources.

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