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Table 2.

Twelve SPHerIC survey protocluster candidates with the highest surface densities of IRAC red sources surrounding a BRCG

Name RA Dec σ1′
hh:mm:ss.ss dd:mm:ss.s arcmin−2
SPHerIC J053020−495751 05:30:20.11 −49:57:51.1 26.42
SPHerIC J102840+432405 10:28:40.91 +43:24:05.2 25.78
SPHerIC J000747−360958 00:07:47.75 −36:09:58.7 24.83
SPHerIC J022635−441345 02:26:35.39 −44:13:45.1 24.51
SPHerIC J143346+121257 14:33:46.98 +12:12:57.1 23.87
SPHerIC J000042−012627a 00:00:42.50 −01:26:27.8 23.55
SPHerIC J173317+522418 17:33:17.65 +52:24:18.6 22.60
SPHerIC J134329+505905 13:43:29.65 +50:59:06.0 22.28
SPHerIC J022115−535903 02:21:15.86 −53:59:03.8 21.96
SPHerIC J082108+763356 08:21:08.60 +76:33:56.5 21.96
SPHerIC J145417+624103 14:54:17.68 +62:41:03.3 21.33
SPHerIC J054936−252504 05:49:36.81 −25:25:04.8 21.01

Notes. All of these candidates are 4σ above the mean surface density derived from SpUDS and are rank ordered by surface density (not RA). (a)Discussed in Flores-Cacho et al. (2016).

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