Table G.2
C1 candidate clusters not yet spectroscopically confirmed with official name, coordinates (J2000), guessed redshift, number of available spectroscopic redshifts along the line of sight, and X-ray flux and uncertainty as in XXL Paper II and in the [0.5–2] keV band.
| IAU name | α | δ | z | Ngal | F60 | Flag |
|---|---|---|---|---|---|---|
| 10−15 | ||||||
| deg | deg | erg s−1 cm−2 | ||||
| 3XLSS J021210.6-061235 | 33.044 | −6.210 | 0.426 | 2 | 28 ± 5 | l |
| 3XLSS J021825.9-045947 | 34.608 | −4.997 | 1.132 | 1 | 4 ± 1 | |
| 3XLSS J232704.6-525831 | 351.769 | −52.975 | 0.583 | 1 | 26 ± 4 | l |
| 3XLSS J233116.6-550737 | 352.819 | −55.127 | 1.296 | 1 | 5 ± 2 | |
| 3XLSS J020604.1-072432 | 31.517 | −7.409 | 0.563 | P | 11 ± 3 | |
| 3XLSS J020720.0-060936 | 31.833 | −6.160 | 0.460 | P | 5 ± 3 | |
| 3XLSS J021803.5-055524 | 34.514 | −5.923 | 0.450 | P | 29 ± 5 | l |
| 3XLSS J022043.7-030106 | 35.182 | −3.019 | 0.160 | P | 18 ± 5 | l |
| 3XLSS J231609.8-541617 | 349.041 | −54.272 | 0.288 | P | 7 ± 2 | |
| 3XLSS J232713.5-560337 | 351.806 | −56.061 | 0.9201 | P | 22 ± 3 | l |
| 3XLSS J232801.9-545545 | 352.008 | −54.929 | 0.960 | P | 21 ± 3 | l |
| 3XLSS J233407.0-523709 | 353.529 | −52.619 | 0.560 | P | 14 ± 3 | l |
| 3XLSS J233531.3-543511 | 353.881 | −54.586 | 0.866 | P | 31 ± 4 | l |
| 3XLSS J233706.8-541910 | 354.279 | −54.320 | 0.524 | P | 14 ± 3 | l |
| 3XLSS J233948.0-541126 | 354.950 | −54.191 | 0.738 | P | 10 ± 3 | |
| 3XLSS J234137.0-545208 | 355.404 | −54.869 | 0.597 | P | 13 ± 3 | l |
| 3XLSS J234154.7-550746 | 355.478 | −55.129 | 0.630 | P | 12 ± 3 | |
| 3XLSS J021604.6-032625 | 34.021 | −3.440 | 0 | 16 ± 3 | l | |
| 3XLSS J022157.6-034002 | 35.490 | −3.666 | 0 | 9 ± 1 | ||
| 3XLSS J022732.0-031456 | 36.883 | −3.248 | 0 | 2 ± 1 | ||
| 3XLSS J231731.6-551424 | 349.382 | −55.240 | 0 | 27 ± 4 | l | |
| 3XLSS J231639.5-553418 | 349.165 | −55.572 | 0 | 20 ± 3 | l | |
| 3XLSS J232624.8-524209 | 351.603 | −52.703 | 2 | 0 | 21 ± 3 | l |
| 3XLSS J234550.2-535247 | 356.459 | −53.880 | 0 | 8 ± 3 | ||
Notes. The first list is for cluster candidates with not enough spectroscopic redshifts to be confirmed, the second list for cluster candidates with no spectroscopic redshift but a photometric redshift estimate, and the third list for cluster candidates with neitherspectroscopic nor photometric redshift estimate. P in the fifth column means that we only have a photometricredshift estimate. An empty fourth column means that we have no estimate at all of the redshift. (1) Photometric redshift for 3XLSS J232713.5-560337 is given in Suhada et al. (2012). (2)3XLSS J232624.8-524210 is heavily polluted by a very bright star so its C1 classification is uncertain and the determination of a photometric redshift was impossible. In the last column (flag), l means that the considered cluster is brighter than the reference flux completeness limit (~1.3 × 10−14 erg s−1 cm−2).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.