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Table 2
For the Planck candidate new clusters not yet confirmed at the time of submission, external information from RASS.
| Name | RASS | Distance to | S/N of | S/N of RASS | Note |
| association | source (arcmin) | RASS source | in Planck aperture | ||
|
|
|||||
| PLCKESZ G115.71+17.52 | BSC | 0.17 | 8.7 | 8.5 | Possible contamination by dust emission |
| PLCKESZ G121.11+57.01 | FSC | 1.72 | 2.9 | 4.1 | Possible association with WHL J125933.4+600409 from Wen et al. (2009), z = 0.33 |
| PLCKESZ G189.84-37.24 | None | – | – | 1.3 | Low reliability, high level of contamination by Galactic emission |
| PLCKESZ G225.92-19.99 | FSC | 1.11 | 2.5 | 6.7 | With XMM-Newton and HST pointed observations |
| PLCKESZ G255.62-46.16 | FSC | 0.9 | 2.7 | 3.8 | With ESO and Suzaku pointed observations |
| PLCKESZ G264.41+19.48 | BSC | 1.22 | 4.6 | 5.7 | |
| PLCKESZ G283.16-22.93 | FSC | 0.54 | 3.6 | 4.2 | |
| PLCKESZ G304.84-41.42 | BSC | 0.55 | 3.6 | 5.1 | With ESO pointed observations |
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