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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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