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Table A.1

List of new 37 PSZ2 clusters confirmed using the SDSS DR12 data.

ID Planck name R. A. Decl. Cen. zphot zspec zspec(BCG) Nspec rmag(BCG) R Comments
34 PSZ2 G009.04+31.09 16:18:26.70 –04:11:11.06 1 0.25 0 0 0 17.42 31 ± 5.5 WHL J161826.7–041111
68 PSZ2 G021.02–29.04 20:20:28.21 –22:25:14.92 1 0.32 0.305a 0 2a 17.74 15 ± 3.8 WHL J202028.2–222515
115 PSZ2 G032.31+66.07 14:37:24.97 +24:23:54.96 2 0.62 0.609 –1 6 WHL J143725.0+242355
161 PSZ2 G044.21+52.13 15:42:50.44 +27:49:52.90 1 0.39 0.378 0.3775 2 18.91 12 ± 3.4 WHL J154250.4+274953
176 PSZ2 G045.96–26.94 20:50:01.00 –01:35:24.30 1 0.20 0 0 0 17.25 10 ± 3.1
277 PSZ2 G066.34+26.14 18:01:06.52 +39:52:06.73 1 0.63 0 0 0 19.96 10 ± 3.1 WHL J180111.8+395138
279 PSZ2 G066.59–58.51 23:07:11.30 –07:31:43.15 1 0.36 0 0 0 18.88 7 ± 2.6 WHL J230711.3–073143
284 PSZ2 G067.21–20.49 21:13:28.88 +18:03:27.47 1 0.31 0 0 0 17.45 5 ± 2.2 WHL J211328.9+180327
293 PSZ2 G069.35–15.58 21:02:41.68 +22:43:13.63 1 0.09 0.094a 0.0958a 2a 14.87 25 ± 5
294 PSZ2 G069.39+68.05 14:21:38.35 +38:21:17.78 2 0.71 0.762 0.762 1 21.23 ClG-J142138.3+382118b
295 PSZ2 G069.47–29.06 21:46:02.16 +14:01:25.90 1 0.36 0 0 0 19.49 11 ± 3.3
330 PSZ2 G077.67+30.59 17:46:50.85 +50:31:11.88 1 0.23 0 0 0 18.07 6 ± 2.4 WHL J174650.9+503112
371 PSZ2 G084.69–58.60 23:36:37.52 –01:27:52.34 1 0.19 0.185 0 2 16.25 7 ± 2.6 WHL J233637.5–012752
381 PSZ2 G086.28+74.76 13:37:53.87 +38:54:06.82 1 0.8 0.699 0.6995 1 21.63
394 PSZ2 G087.39–34.58 22:49:09.53 +19:44:30.50 2 0.7 0.76 –1 1
424 PSZ2 G093.41–16.26 22:24:07.25 +37:58:30.46 1 0.26 0 0 0 17.37 7 ± 2.6 WHL J222407.2+375831
432 PSZ2 G094.31–11.31 22:12:58.51 +42:35:02.26 1 0.24 0 0 0 16.62 13 ± 3.6
483 PSZ2 G100.22+33.81 17:13:45.53 +69:21:48.07 2 0.62 0 –1 0
620 PSZ2 G125.84–18.72 01:06:55.84 +44:06:05.81 2 0.19 0 –1 0 16 ± 4 WHL J010709.2+440918.
624 PSZ2 G126.36–19.11 01:09:19.54 +43:37:40.78 1 0.22 0 0 0 16.37 10 ± 3.1 WHL J010919.5+433741
628 PSZ2 G126.72–21.03 01:10:25.02 +41:41:18.81 1 0.22 0 0 0 15.83 5 ± 2.2 WHL J011025.0+414119
644c PSZ2 G130.64+37.16 10:47:45.54 +77:59:56.67 1 0.44 0 0 0 19.98 6 ± 2.4 WHL J104745.5+775957
644c PSZ2 G130.64+37.16 10:46:29.31 +78:07:44.06 1 0.24 0 0 0 17.10 7 ± 2.6 WHL J104629.2+780744
646 PSZ2 G131.15–14.72 01:38:42.22 +47:22:35.27 2 0.24 0 –1 0 31 ± 5.5 WHL J013846.1+472236.
681 PSZ2 G139.00+50.92 11:20:16.97 +63:14:59.87 2 0.6 0 –1 0
732 PSZ2 G150.64–14.21 03:17:04.20 +40:41:33.22 1 0.22 0 0 0 16.86 10 ± 3.1 WHL J031704.2+404133
810 PSZ2 G171.08–80.38 01:21:53.35 –20:33:26.69 1 0.33 0 0 0 17.36 6 ± 2.4 WHL J012153.4–203327
831 PSZ2 G177.03+32.64 08:13:20.93 +43:12:36.83 1 0.16 0.1428 0.143 6 16.85 20 ± 4.4 WHL J081320.9+431237
836 PSZ2 G179.45–43.92 03:19:18.34 +02:05:35.43 1 0.34 0 0 0 16.91 5 ± 2.2 WHL J031918.3+020535
863 PSZ2 G186.50–13.45 05:11:52.85 +16:13:36.29 1 0.25 0 0 0 16.6 9 ± 3 WHL J051152.9+161336
1049 PSZ2 G231.41+77.48 12:00:26.54 +22:34:19.55 1 0.35 0.346 0.3469 2 18.55 10 ± 3.1 WHL J120026.5+223420
1074 PSZ2 G237.68+57.83 10:53:17.80 +10:52:37.13 1 0.7 0 –1 0
1244 PSZ2 G269.02+46.30 11:19:07.43 –10:22:57.81 2 0.12 0 –1 0 8 ± 2.8
1254c PSZ2 G270.78+36.83 11:04:06.99 –19:13:47.88 1 0.22 0 0 0 16.88 12 ± 3.4 WHL J110407.0–191348
1254c PSZ2 G270.78+36.83 11:04:21.03 –19:14:18.12 1 0.52 0 0 0 19.59 18 ± 4.2 WHL 110417.9–191409
1255 PSZ2 G270.88+37.23 11:05:04.58 –18:56:38.66 1 0.23 0 0 0 16.62 15 ± 3.8 WHL J110504.6–185639
1262c PSZ2 G271.53+36.41 11:05:25.72 –19:54:19.84 1 0.48 0 0 0 17.84 5 ± 2.2 WHL J110525.7–195420
1262c PSZ2 G271.53+36.41 11:05:19.71 –19:59:15.61 2 0.50 0 –1 0 6 ± 2.4 WHL J110519.6–195852
1465 PSZ2 G310.81+83.91 12:55:18.02 +21:02:31.22 1 0.44 0.429 0.4288 2 19.54 5 ± 2.4 PSZ1 G311.76+83.91
1548 PSZ2 G328.96+71.97 13:23:27.81 +10:46:43.71 2 0.09 0.092 –1 10 10 ± 3.1

Notes. The first two columns are the index number and the official name of the SZ target in the PSZ2 catalogue. The J2000 coordinates (cols. 3 and 4) correspond to the BCG position or geometrical centre (labelled as Cen = 1 or Cen = 2 in Col. 5, respectively) of the identified counterpart. Column 6 shows the photometric redshift of the cluster. Columns 7, 8, and 9 show (if available) the mean spectroscopic redshift, spectroscopic redshift of the BCG (in the case of absence of the apparent BCG we write “–1”), and the number of galaxies with spectroscopic measurements. Column 10 provides the r magnitude (corrected for extintion) of the BCG. Column 11 presents optical richness of the cluster and its error, where possible (see Sect. 4.4 for details). The last column includes the source name in Wen et al. (2012).

(a)

Spectroscopic redshift obtained from optical follow-up observations with the WHT telescope. No spectroscopic SDSS data available.

(b)

Additional analysis presented in Buddendiek et al. (2015).

(c)

Multiple optical detection.

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