Table 2
ERCSC sources at 545 GHz and their H-ATLAS 500 μm counterparts inside a 4.47 arcmin radius circle around the ERCSC position.
| ID | Name | RA (deg) | Dec (deg) | S545 GHz (Jy) | ΔS545 GHz | EXT | CIRRUS | H-ATLAS ID | Other ID | S500 μm (Jy) | ΔS500 μm (Jy) | zspec | D (arcmin) |
|
|
|||||||||||||
| 3 | G224.70+24.61 | 129.951 | 1.422 | 1.543 | 0.517 | 0 | 0.156 | ||||||
| 6 | G226.97+26.25 | 132.394 | 0.458 | 2.185 | 0.647 | 1 | 0.109 | ||||||
| 8 | G227.27+24.71 | 131.198 | –0.550 | 3.718 | 1.536 | 1 | 0.125 | ||||||
| 9 | G227.57+24.56 | 131.215 | –0.863 | 4.234 | 1.194 | 1 | 0.125 | ||||||
| 10 | G227.77+30.23 | 136.181 | 1.869 | 4.554 | 1.168 | 1 | 0.078 | ||||||
| 29 | G230.17+32.05 | 138.809 | 1.055 | 1.191 | 0.463 | 0 | 0.141 | ||||||
| 13 | G231.44+32.10 | 139.420 | 0.174 | 1.410 | 0.389 | 0 | 0.125 | ||||||
| 18 | G270.59+58.54 | 176.648 | –0.199 | 1.358 | 0.610 | 0 | 0.031 | J114637.9-001132 | G12H29 | 0.298 | 0.008 | 3.259 | 0.746 |
| 20 | G277.36+59.21 | 180.094 | –1.097 | 4.546 | 0.419 | 0 | 0.047 | J120023.2-010600 | NGC 4030 | 5.661 | 0.052 | 0.0048 | 0.229 |
| 21 | G345.12+54.85 | 215.603 | –0.381 | 1.151 | 0.415 | 0 | 0.016 | J142223.4-002313 | NGC 5584 | 1.441 | 0.033 | 0.0055 | 0.460 |
| 24 | G351.01+52.12 | 220.047 | –0.292 | 2.213 | 0.524 | 0 | 0.078 | J144011.1-001725 | NGC 5713 | 2.278 | 0.035 | 0.0063 | 0.141 |
| 25 | G351.21+51.96 | 220.242 | –0.327 | 1.275 | 0.439 | 0 | 0.078 | J144056.2-001906 | NGC 5719 | 1.817 | 0.073 | 0.0057 | 0.729 |
| 26 | G353.14+54.45 | 219.414 | 2.290 | 1.551 | 0.433 | 0 | 0.062 | J143740.9+021729 | NGC 5690 | 2.210 | 0.046 | 0.0855 | 0.409 |
| 28 | G354.97+52.95 | 221.236 | 1.956 | 3.456 | 0.534 | 0 | 0.062 | J144455.9+015719 | NGC 5746 | 2.686 | 0.081 | 0.0058 | 0.204 |
Notes. Planck flux densities and their associated errors are taken from the ERCSC GAUFLUX column.Only the H-ATLAS sources with flux density S500 μm ≳ 0.3 Jy have been included in the table (blank spaces mean that no H-ATLAS source brighter than 0.3 Jy at 500 μm are associated to the ERCSC detection). In the case of G270.59+58.54 the redshift refers to the strongly lensed galaxy G12H29. The ID numbers correspond to the counterparts of these objects in Table 1, except for the case of G230.17+32.05 which has no clear counterpart in that table.
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