Table 1.
Galaxy group and cluster members of the Perseus-Pisces SC.
Name | RA | Dec | Redshift | Flux | Err. | LX | m200 | rout | nH | R | Alt. name |
---|---|---|---|---|---|---|---|---|---|---|---|
RXCJ2332.5+2355 | 353.1303 | 23.9266 | 0.0173 | 1.6108 | 17.50 | 0.0143 | 0.266 | 7.5 | 4.4 | D | UGC 12655 |
RXCJ0015.5+1720 | 3.8764 | 17.3350 | 0.0181 | 1.9179 | 35.80 | 0.0181 | 0.308 | 8.0 | 4.0 | D | NGC 57 |
RXCJ0018.3+3003 | 4.5984 | 30.0630 | 0.0223 | 2.5900 | 20.10 | 0.0374 | 0.484 | 7.5 | 5.5 | D | NGC 71 |
RXCJ0021.0+2216 | 5.2628 | 22.2754 | 0.0193 | 5.1874 | 25.50 | 0.0464 | 0.554 | 16.0 | 4.2 | D | SRGb063 (a), PPS 62 (b) |
RXCJ0107.2+3224 | 16.8206 | 32.4067 | 0.0174 | 6.6932 | 10.30 | 0.0512 | 0.590 | 14.5 | 5.2 | C | NGC 383 |
RXCJ0110.9+3308 | 17.7425 | 33.1486 | 0.0177 | 2.2140 | 20.00 | 0.0277 | 0.404 | 5.0 | 5.9 | C | NGC 410 |
RXCJ0123.1+3327 | 20.7971 | 33.4612 | 0.0147 | 6.0909 | 18.00 | 0.0416 | 0.519 | 9.0 | 5.3 | C | NGC 499 |
RXCJ0123.6+3315 | 20.9041 | 33.2516 | 0.0166 | 17.1433 | 15.00 | 0.1523 | 1.159 | 10.0 | 5.3 | C | NGC 507 |
RXCJ0152.7+3609 | 28.1942 | 36.1509 | 0.0161 | 71.6749 | 4.50 | 0.4227 | 2.185 | 38.0 | 5.5 | C | A 262 |
RXCJ0200.2+3126 | 30.0704 | 31.4346 | 0.0167 | 4.0825 | 16.00 | 0.0308 | 0.430 | 11.0 | 5.5 | C | NGC 777 |
RXCJ0222.7+4301 | 35.6965 | 43.0182 | 0.0212 | 7.0947 | 20.80 | 0.0910 | 0.841 | 9.0 | 9.1 | C | UGC 1841 |
RXCJ0238.7+4138 | 39.6977 | 41.6478 | 0.0153 | 2.3705 | 21.20 | 0.0130 | 0.253 | 14.5 | 7.6 | C | NGC 996 |
RXCJ0249.5+4658 | 42.3899 | 46.9768 | 0.0274 | 2.3755 | 19.40 | 0.0433 | 0.530 | 11.5 | 13.4 | E | IC 0256/0257 |
RXCJ0254.4+4134 | 43.6214 | 41.5764 | 0.0172 | 110.5048 | 2.20 | 0.9477 | 3.601 | 17.5 | 9.2 | C | AWM7 (NGC 1129) |
RXCJ0300.7+4428 | 45.1791 | 44.4675 | 0.0302 | 41.8408 | 4.00 | 0.9475 | 3.578 | 17.5 | 14.9 | F | CIZAJ0300.7+4427 |
RXCJ0309.9+4207 | 47.4981 | 42.1255 | 0.0300 | 1.4685 | 19.70 | 0.0316 | 0.434 | 11.0 | 12.7 | E | UGC 2562 |
RXCJ0310.3+4250 | 47.5755 | 42.8488 | 0.0314 | 2.6345 | 19.00 | 0.0668 | 0.681 | 9.0 | 16.2 | F | |
RXCJ0319.7+4130 | 49.9498 | 41.5149 | 0.0179 | 688.3633 | 0.90 | 7.7309 | 13.227 | 17.5 | 15.7 | C | A 426 (Perseus) |
RXCJ0348.1+4212 | 57.0337 | 42.2145 | 0.0174 | 3.3776 | 17.20 | 0.0324 | 0.443 | 7.5 | 23.7 | C | MCG +07−08−033 |
RXCJ0421.8+3607 | 65.4689 | 36.1200 | 0.0208 | 11.6173 | 10.10 | 0.1279 | 1.038 | 14.5 | 26.2 | C | UGC 3021 |
RXCJ0450.0+4501 | 72.5146 | 45.0242 | 0.0210 | 69.6988 | 5.50 | 0.8256 | 3.300 | 17.5 | 67.9 | C | 3C 129 |
RXCJ0547.2+5052 | 86.8160 | 50.8786 | 0.0263 | 9.1313 | 11.70 | 0.1490 | 1.139 | 17.0 | 17.8 | E | UGC 3355 |
Notes. The flux is in units of 10−12 erg s−1 cm−2 in the 0.1−2.4 keV band, and the error in the following column is in percent. The X-ray luminosity, LX, is in units of 1044 erg s−1 for 0.1−2.4 keV within r500; m200 is the cluster mass estimated from the LX–mass relation within r200; rout is the radius out to which the X-ray luminosity is detected in the RASS; and nH is the interstellar column density in the line of sight in units of 1020 cm−2. R indicates to which part of the Perseus-Pisces SC the member belongs: C = core, D = other members z ≤ 0.025, E = members with z = 0.025 − 0.03, and F = members at z > 0.03. In the last column we provide alternative names of the systems; groups are often designated by the name of the central dominant galaxy.
Group described in Mahdavi et al. (2000),
system in the Perseus-Pisces Group Survey of Trasart-Battistani (1998).
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