In Sunyaev-Zeldovich (SZ) cluster cosmology, accurately determining cluster masses is crucial for constraining cosmological parameters through cluster number counts. As the mass is not an observable, a scaling relation is needed to link cluster masses to the integrated Compton parameter Y, i.e., the SZ observable, to exploit data from large millimeter surveys. Former cosmological results use a scaling relation obtained with clusters at low redshift (z < 0.5) observed in X-ray and in SZ at an angular resolution above 1 arcminute. The SZ large program (LPSZ) of the NIKA2 collaboration uses a sample of clusters at intermediate to high redshift (from z = 0.5 to z = 0.9) observed at similarly high-angular resolution both in SZ and in X-ray. We present the SZ-Mass scaling relation parameters calibrated thanks to the LPSZ data.

The SZ-Mass scaling relation with the NIKA2 SZ large program / Moyer-Anin, A., Adam, R., Ade, P., Ajeddig, H., Amarantidis, S., André, P., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Béthermin, M., Bolliet, B., Bongiovanni, A., Bounmy, J., Bourrion, O., Calvo, M., Catalano, A., Chérouvrier, D., De Petris, M., et al.. - In: EPJ WEB OF CONFERENCES. - ISSN 2100-014X. - 353:(2026), pp. 1-6. [10.1051/epjconf/202635301011]

The SZ-Mass scaling relation with the NIKA2 SZ large program

De Petris, M.;Pisano, G.;
2026

Abstract

In Sunyaev-Zeldovich (SZ) cluster cosmology, accurately determining cluster masses is crucial for constraining cosmological parameters through cluster number counts. As the mass is not an observable, a scaling relation is needed to link cluster masses to the integrated Compton parameter Y, i.e., the SZ observable, to exploit data from large millimeter surveys. Former cosmological results use a scaling relation obtained with clusters at low redshift (z < 0.5) observed in X-ray and in SZ at an angular resolution above 1 arcminute. The SZ large program (LPSZ) of the NIKA2 collaboration uses a sample of clusters at intermediate to high redshift (from z = 0.5 to z = 0.9) observed at similarly high-angular resolution both in SZ and in X-ray. We present the SZ-Mass scaling relation parameters calibrated thanks to the LPSZ data.
2026
astrophysical observations; cosmology; SZ effect; galaxy clusters
01 Pubblicazione su rivista::01a Articolo in rivista
The SZ-Mass scaling relation with the NIKA2 SZ large program / Moyer-Anin, A., Adam, R., Ade, P., Ajeddig, H., Amarantidis, S., André, P., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Béthermin, M., Bolliet, B., Bongiovanni, A., Bounmy, J., Bourrion, O., Calvo, M., Catalano, A., Chérouvrier, D., De Petris, M., et al.. - In: EPJ WEB OF CONFERENCES. - ISSN 2100-014X. - 353:(2026), pp. 1-6. [10.1051/epjconf/202635301011]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1769084
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