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Table 2.

Coordinates and observed photometry of the selected z ≥ 7.5 candidates.

ID RA Dec ID Y J H Ks [3.6] [4.5] Flag (a)
CLASSIC [J2000] [J2000] Farmer [mag] [mag] [mag] [mag] [mag] [mag]
234500 10:02:12.08 01:38:20.22 153872 > 24.8 ...
241443 09:58:00.45 01:38:46.82 228669 1
336101 10:00:32.32 01:44:31.22 499535 ...
403992 10:01:45.04 01:48:28.42 214940 ...
441697 09:57:39.01 01:50:40.05 598190 > 26.7 1
428351 10:00:58.48 01:49:55.97 615402 DB
442053 09:58:32.63 01:50:43.59 711973 > 25.5 DB
485056 10:00:17.89 01:53:14.39 184348 > 25.1 ...
545752 09:57:23.39 01:56:45.93 758856 1
564423 10:00:31.87 01:57:50.12 78629 > 26.6 ...
631862 09:57:42.84 02:01:39.64 747154 ...
720309 09:59:10.82 02:06:41.96 859236 > 26.4 ...
720309 (b) ... ... ... > 26.9 ... ... ...
724872 10:02:52.10 02:06:57.91 729770 D
784810 10:01:47.48 02:10:15.43 749805 > 26.5 ...
852845 09:58:50.94 02:13:55.09 371044 ...
859061 10:00:19.59 02:14:13.28 443686 > 26.6 B
978062 09:57:47.90 02:20:43.55 764263 > 26.7 ...
984164 09:57:18.00 02:21:05.90 774509 > 26.4 2
1055131 09:57:54.25 02:25:08.42 518572 > 26.3 ...
1103149 09:57:54.69 02:27:54.95 71035 ...
1151531 10:02:12.54 02:30:45.84 776124 ...
1209618 10:00:47.53 02:34:04.50 270250 > 26.8 ...
1212944 10:01:56.33 02:34:16.22 391218 ...
1274544 09:58:12.23 02:37:52.34 50411 D
1297232 09:57:24.53 02:39:13.18 292281 2
1313521 09:57:35.64 02:40:12.09 454321 > 26.4 2B
1346929 10:00:30.65 02:42:09.10 764277 > 26.7 ...
1352064 09:57:32.07 02:42:25.56 740295 2
1356755 09:57:25.45 02:42:41.22 9881 > 26.4 ...
1371152 10:00:15.97 02:43:32.91 247885 > 26.7 ...
1409328 09:59:17.15 02:45:48.22 666370 ...
1412106 09:57:21.36 02:45:57.47 331814 > 26.2 2

Notes. The first columns indicate the ID and coordinates from the CLASSIC catalogue. The other columns give the photometry from The Farmer catalogue, corrected for Milky Way extinction and systematic zeropoint offsets. The upper-limits correspond to the 3σ depth of the image at the source coordinates (10σ for IRAC), for sources with S/N < 1. (a)The flags are the following. 1: outside the HSC ultra-deep region, 2: outside the IRAC SPLASH region, B: blended, D: inside the UltraVISTA deep stripe. (b)UltraVISTA photometry measured on a new stack not affected by the contribution of a potential cross-talk artefact (see Sect. 3.4).

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