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Table A.1.

Radio sources found within the group, presented together with their multiwavelength properties (counterparts within 3″ radius) available in the literature (see notes below).

10913 44 4092 1549 10366 633 528
Ra 150.1179 150.1104 150.1461 150.1080 150.1386 150.1602 150.1235
Dec 2.6843 2.7083 2.6985 2.6955 2.7030 2.6993 2.6717
Spectroscopic
Redshift 0.3491 0.3506 0.3505 0.3492 0.354 0.3044 0.345

Radio properties (Detected / Flux density [mJy] / Multi)

YES / YES / YES / YES / YES / YES / YES /
3 GHz (VLA) 32.09 / 2.3 ± 0.1 / 0.028 ± 0.003 / 0.071 ± 0.004 / 0.011 ± 0.002 / 0.121 ± 0.007 / 0.152 ± 0.008 /
1 0 0 0 0 0 0

Xray properties (Detected / Full X-ray (2-10 keV) Flux [erg/s/cm2])

Chandra (2016) YES / 3.15 × 10−15 YES / 4.6 × 10−15 NO / - NO / - NO / - NO / - YES / 3.93 × 10−15

Photometric properties of optical counterparts

CLASSIC ID - 1358068 1352485 1346601 1351402 1353634 -
HSC i mag Aper2 - 19.322 ± 0.001 19.690 ± 0.002 19.944 ± 0.002 21.764 ± 0.004 19.815 ± 0.002 -
COSMOS2015 ID 901584 923481 921175 920711 925241 923235 902831
SC i+ mag Aper2 18.826 ± 0.002 19.391 ± 0.003 19.742 ± 0.004 19.991 ± 0.003 21.83 ± 0.01 19.883 ± 0.004 19.922 ± 0.004
ACS F814W mag 17.310 ± 0.001 18.350 ± 0.001 19.330 ± 0.001 19.360 ± 0.001 21.310 ± 0.007 18.990 ± 0.002 19.050 ± 0.002

Notes. First two, 10913 and 44, are tailed radio galaxies. The radio data were adopted from the source catalog at 3 GHz (Smolčić et al. 2017b), X-ray properties are from Chandra catalog of point sources (Civano et al. 2016), and optical/NIR photometry data from CLASSIC (Weaver et al. 2022) and COSMOS2015 (Laigle et al. 2016) multiwavelength photometry catalogs. HSC i band magnitudes were adopted from CLASSIC, and SC i+ and HST-ACS-F814W magnitudes from COSMOS2015 catalog. Only selected (relevant) properties are presented here, and for the others one should refer to the corresponding catalogs. Errors are provided when available. ( † )From Khostovan et al. (2025). ( ★ )For details on X-ray detections (full/soft/hard) see the analysis of X-ray point sources within the group, Table A.3.

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