Clusters of galaxies are powerful cosmological probes, and the thermal Sunyaev Zel’dovich (tSZ) effect provides an efficient method for their detection. High-angular-resolution observations, such as those provided by the NIKA2 camera on the IRAM 30-m telescope, are essential to target low mass and high-redshift clusters. We performed a blind search for galaxy clusters in the COSMOS field using 150 GHz data from the NIKA2 Cosmological Legacy Survey. We applied a matched-filter technique based on a universal pressure profile to extract cluster candidates. The purity and completeness of the sample were assessed using realistic simulations. We detected 16 cluster candidates above an S/N of 4, eight of which have confirmed counterparts.
Blind detection of galaxy clusters in the COSMOS field via the SZ effect / Chérouvrier, D., Adam, R., Ade, P., Ajeddig, H., Amarantidis, S., André, P., Aussel, H., Barrena, R., Beelen, A., Benoît, A., Berta, S., Béthermin, M., Bongiovanni, A., Bounmy, J., Bourrion, O., Bing, L.-J., Calvo, M., Catalano, A., De Petris, M., Désert, F.X., et al.. - In: EPJ WEB OF CONFERENCES. - ISSN 2100-014X. - 353:(2026), pp. 1-6. [10.1051/epjconf/202635301003]
Blind detection of galaxy clusters in the COSMOS field via the SZ effect
De Petris, M.;Pisano, G.;
2026
Abstract
Clusters of galaxies are powerful cosmological probes, and the thermal Sunyaev Zel’dovich (tSZ) effect provides an efficient method for their detection. High-angular-resolution observations, such as those provided by the NIKA2 camera on the IRAM 30-m telescope, are essential to target low mass and high-redshift clusters. We performed a blind search for galaxy clusters in the COSMOS field using 150 GHz data from the NIKA2 Cosmological Legacy Survey. We applied a matched-filter technique based on a universal pressure profile to extract cluster candidates. The purity and completeness of the sample were assessed using realistic simulations. We detected 16 cluster candidates above an S/N of 4, eight of which have confirmed counterparts.| File | Dimensione | Formato | |
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