Table A.1.
Completeness of X-ray cluster catalogs. Columns are: 1. Full name of the catalog, 2. Acronym of the catalog, 3. Percentage of the total sky area observed by the survey, 4. Redshift range, 5. Limiting observed flux FX, 6. Completeness for flux > FX, and 7. M200c mass limit at the median redshift, and at z=0.5-1, calculated following Pratt et al. (2009). We indicate the redshift (or the redshift range) in parenthesis.
| Name | Acronym | Area | Redshift range | FX | Comp. | M200c limit |
|---|---|---|---|---|---|---|
| % of sky | erg/cm2/s | % | M⊙ | |||
| MCXC: ROSAT | ||||||
| ROSAT-ESO Flux-Limited X-Ray | REFLEXa | 33 | 0< z< 0.3 | 3 ⋅ 10−12 | 100 | 1013.9 (0.075) |
| 1015.1 − 15.6 (0.5-1) | ||||||
| Northern ROSAT All-Sky | NORASb | 41 | 0< z< 0.3 | 3 ⋅ 10−12 | 50 | 1013.9 (0.075) |
| Galaxy Cluster Survey | 1015.1 − 15.6 (0.5-1) | |||||
| ROSAT Brightest Cluster Sample | BCSc | 41 | 0< z< 0.3 | 4.4 ⋅ 10−12 | 90 | 1013.9 (0.075) |
| 1015.1 − 15.6 (0.5-1) | ||||||
| Catalog of clusters in the region of | SGPd | 8 | 0< z< 0.3 | 3 ⋅ 10−12 | 100 | 1013.9 (0.075) |
| 1 ster. around the south galactic pole | 1015.1 − 15.6 (0.5-1) | |||||
| ROSAT north ecliptic pole survey | NEPe | 0.2 | 0< z< 0.8 | 2.0 ⋅ 10−14 | 100 | 1013.9 (0.200) |
| 1014.5 − 15.0 (0.5-1) | ||||||
| Massive Cluster Survey | MACSf | 55 | 0.3< z< 0.6 | 2 ⋅ 10−12 | 93 | 1013.9 (0.370) |
| 1014.5 − 15.0 (0.5-1) | ||||||
| < 2 ⋅ 10−12 | 59 | |||||
| MCXC: Serendipitous surveys | ||||||
| 160 Square Degree ROSAT Survey | 160SDg | 3.8 | 0< z< 0.7 | 1.4 ⋅ 10−14 | 100 | 1013.6 (0.250) |
| 1014.3 − 14.8 (0.5-1) | ||||||
| 400 Square Degree ROSAT PSPC | 400SDh | 9.5 | 0< z< 0.7 | 1.4 ⋅ 10−14 | 100 | 1013.6 (0.200) |
| Galaxy Cluster Survey | 1014.5 − 15.0 (0.5-1) | |||||
| Southern Serendipitous High-redshift | SHARCi | 0.4 | 0< z< 0.7 | 4.6 ⋅ 10−14 | 100 | 1013.6 (0.340) |
| Archival ROSAT Cluster survey | 1014.5 − 15.0 (0.5-1) | |||||
| Extended Medium-Sensitivity Survey | EMSSj | 1.8 | 0< z< 0.7 | 5 ⋅ 10−14..3 ⋅ 10−12 | 100 | 1013.6 (0.115) |
| Distant Cluster Sample | 1014.5 − 15.0 (0.5-1) | |||||
| Wide Angle ROSAT Pointed Survey | WARPSk | 1.3 | 0< z< 0.9 | 6.5 ⋅ 10−14 | 100 | 1013.6 (0.284) |
| Distant Cluster Sample | 1014.2 − 14.7 (0.5-1) | |||||
| eROSITA Final Equatorial-Depth Survey | eFEDSl | 3.3 | 0< z< 1.3 | 1 ⋅ 10−14 | 40 | 1013.8 (0.353) |
| 1014.1 − 14.6 (0.5-1) | ||||||
| eRASS1 cosmology cluster samplem | 50 | 0< z< 1.3 | 1.6 ⋅ 10−12 | 80 | 1014.4 (∼0.300) | |
| 1014.1 − 14.6 (0.5-1) |
Notes. aBohringer et al. (2004); bBohringer et al. (2000); cEbeling et al. (1998); dCruddace et al. (2002); eHenry et al. (2006); fEbeling et al. (2001); gMullis et al. (2003); hBurenin et al. (2007); iRomer et al. (2000), Burke et al. (2003); jGioia et al. (1990); kPerlman et al. (2002), Horner et al. (2008);lBrunner et al. (2022); mMerloni et al. (2024), Kluge et al. (2024)
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