Open Access

Table 4

Overview of the catalogs analyzed with eROMaPPer in this work.

Survey Source Cataloged clusters In LS footprint Survey area [deg2]
X-ray selected
eRASS1 Bulbul et al. (2024) & this work 12 247 12 247 13 116
CODEX Finoguenov et al. (2020) 10 382 10079 10 269
MCXC Piffaretti et al. (2011) 1743 1477 ~all sky
NORAS Böhringer et al. (2017) 378 344 13 519
XXL Adami et al. (2018) 302 299 50
XCLASS Koulouridis et al. (2021) 1559 1433 269

SZ selected
ACT Hilton et al. (2021) 4195 4044 13 211
SPT Bleem et al. (2015) 677 656 2500
PSZ2 Planck Collaboration XXVII (2016) 1653 1207 ~all sky

Optically selected
LS DR10 south grz This work 112 609 112 609 19 342
LS DR10 south grzw1 This work 273 150 273 150 19 342
LS DR10 south griz This work 91 790 91 790 15 326
LS DR10 south grizw1 This work 242 044 242044 15 326
LS DR9 north grz This work 27 516 27 516 5068
LS DR9 north grzw1 This work 93 227 93 227 5068
ACO Abell et al. (1989) 5250 4635 ~all sky
DESY1 Abbott et al. (2020) 6729 6724 1437

Notes. The survey area was calculated from the high-resolution HEALPix maps for eRASS1 and the optically selected LS catalogs or taken from the catalog paper in the source column. Three catalogs have survey areas that cover approximately the full sky but (partly) exclude the Galactic plane, as shown in Fig. 9. A richness cut of λnorm > 16 and a redshift constraint zλ < zvlim were applied to the LS DR9 north and LS DR10 south catalogs. Although the number of detections is huge, the contamination fraction in these catalogs is not well known.

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.