Exploiting NIKA2/XMM-Newton imaging synergy for intermediate-mass high-z galaxy clusters within the NIKA2 SZ large program

Autor: Kéruzoré, F., Mayet, F., Pratt, G. W., Adam, R., Ade, P., André, P., Andrianasolo, A., Arnaud, M., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Gomez, A., Goupy, J., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Mauskopf, P., Monfardini, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C.

Publikováno v: DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A93. ⟨10.1051/0004-6361/202038933⟩
Universidad de Alicante (UA)

High-resolution mapping of the intra-cluster medium (ICM) up to high redshift and down to low masses is crucial to derive accurate mass estimates of the galaxy cluster and to understand the systematic effects affecting cosmological studies based on g

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96bdd2e0f9579515f3c2b80b2a74c5a3
https://orca.cardiff.ac.uk/id/eprint/137311/1/aa38933-20.pdf