Table 1
Summary of ancillary information used in selecting candidates for XMM observations, and log of the XMM-Newton observations.
| Name | RASZ | DecSZ | S/N | N det | Q SZ | OBSID | Filter | t exp | Clean fraction | Category | Confirmed |
| (deg) | (deg) | (ks EPN) | (EMOS/EPN) | ||||||||
|
|
|||||||||||
| PLCKG348.4−25.5 | 291.257 | −49.426 | 6.12 | 3 | A | 0679180101 | t t t | 10.6 | 1.0/0.9 | PHZ | Y |
| PLCKG329.5−22.7† | 278.270 | −65.570 | 5.84 | 3 | B | 0679181501 | m m t | 8.5 | 1.0/1.0 | ... | Y |
| PLCKG219.9−34.4 | 73.680 | −20.269 | 5.74 | 2 | A | 0679180501 | t t t | 9.5 | 1.0/0.9 | PHZ | Y |
| PLCKG352.1−24.0 | 290.233 | −45.842 | 5.63 | 2 | C | 0679180201 | m m t | 8.5 | 1.0/1.0 | PHZ | Y |
| PLCKG305.9−44.6 | 5.946 | −72.393 | 5.40 | 3 | B | 0679180301 | t t t | 10.1 | 0.4/0.2 | ... | Y |
| PLCKG196.7−45.5† | 55.759 | −8.704 | 5.21 | 3 | B | 0679180401 | m m m | 9.0 | 1.0/0.8 | ... | Y |
| PLCKG208.6−74.4 | 30.044 | −24.897 | 5.01 | 3 | B | 0679180601 | t t t | 2.9 | 0.8/0.8 | ... | Y |
| PLCKG130.1−17.0 | 22.678 | 45.288 | 4.93 | 3 | C | 0679180801 | t t t | 7.5 | 1.0/1.0 | ... | Y |
| PLCKG239.9−40.0 | 71.683 | −37.029 | 4.76 | 3 | B | 0679181001 | t t t | 9.9 | 1.0/1.0 | ... | Y |
| PLCKG310.5 + 27.1 | 201.148 | −35.245 | 4.77 | 2 | B | 0679180901 | t t t | 12.9 | 0.9/0.8 | PHZ | ... |
| PLCKG196.4−68.3 | 34.921 | −19.263 | 4.73 | 2 | B | 0679181101 | t t t | 11.8 | 0.7/0.4 | PHZ | ... |
| PLCKG204.7 + 15.9 | 113.614 | 14.295 | 4.57 | 3 | A | 0679180701 | t t t | 9.4 | 1.0/1.0 | ... | Y |
| PLCKG011.2−40.4 | 315.233 | −33.107 | 4.47 | 1 | C | 0679181201 | t t t | 8.5 | 1.0/1.0 | PHZ | Y |
| PLCKG147.3−16.6 | 44.099 | 40.291 | 4.41 | 3 | B | 0679181301 | t t t | 10.7 | 0.9/0.6 | PHZ | Y |
| PLCKG210.6 + 20.4 | 120.218 | 11.093 | 4.01 | 1 | C | 0679181401 | t t t | 8.5 | 1.0/1.0 | SDSS | ... |
Notes. Column (1): Planck source name. Columns (2) and (3): right ascension and declination of the Planck source (J2000). Columns (4) and (5): signal-to-noise ratio of the Planck cluster candidate detection with the MMF3 algorithm in the Planck-maps, and number of methods blindly detecting the candidate. Column (6): quality grade of the SZ detection (A is best). Columns (7)−(10): XMM-Newton observation identification number, filter used, on-source exposure time with the EPN camera, and fraction of useful time after cleaning for periods of high background due to soft proton flares (EMOS and EPN camera, respectively). Column (11): category resulting from the pre-selection of the candidates. Column (12): confirmed clusters are flagged.
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