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Table 1.

IDs, SExtractor segmentation numbers, photometric and spectroscopic redshifts, stellar masses and SFRs of group member galaxies.

CANDELS ID 3DHST Seg. zphot zspec log10(M/M, FAST) SFRIR (M yr−1) SFRFAST (M yr−1)
29816 38191 92 1.64±0.24 1.84±0.02 10.03 < 247 < 17.08
30304 38274 78 1.72±0.18 10.50 108±32 < 8.58
30147 38263 90 1.68±0.05 1.85±0.01 10.44 < 169 < 0.67
29630 38497 88 1.95±0.27 1.86±0.01 8.80 < 146 < 0.44
30186 38187 89 1.92±0.10 1.850±0.005 11.32 1810±219 < 168.53
30186 99 10.14 < 2.85
30186 100 9.64 < 0.64
30336 85 1.78±0.21 10.45 < 262 < 27.03
30144 38174 94 1.52±0.16 1.89±0.03 10.29 313±108 < 7.25
29702 38356 87 1.64±0.11 9.83 < 276 < 4.50
30329 38290 79 1.95±0.12 10.76 68±18 < 1.15
28224 38527 83 1.53±0.23 8.88 < 120 < 1.45
38212 95 9.25 < 0.24
96 8.94 < 0.25
180 9.72 < 1.80
38531 181 1.85±0.05 8.53 < 0.12

Notes. zphot are taken from the Stefanon et al. (2017) catalogue, with errors derived from SED fitting in the FIR catalogue. SFRs derived in the FIR catalogue (SFRIR) and using SED fitting (SFRFAST, this work) are labelled accordingly. Stellar masses are taken from our FAST++ fitting, with the 68% errors shown. Some CANDELS IDs appear several times, associated with different segmentation IDs, derived from the higher-resolution imaging (see also Fig. 2). SFRIR shown in bold indicate that the galaxies are detected at S/N > 5 in the FIR regime, and SFRIR are only shown for those galaxies with S/NFIR > 2.5. 3σ upper limits are shown on SFR values (using the errors on the derived SFR, from the FIR catalogue SED fitting or FAST SED fitting, respectively).

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