The XXL Survey XVI. The clustering of X-ray selected galaxy clusters at z similar to 0.3

Author
SERENO, M.
MOSCARDINI, L.
PACAUD, F.
Pierre, M.
PLIONIS, M.
CAPPI, A.
ADAMI, C.
ALTIERI, B.
Birkinshaw, M.
ETTORI, S.
Faccioli, L.
GASTALDELLO, F.
Koulouridis, E.
LIDMAN, C.
LE FEVRE, J. -P.
MAUROGORDATO, S.
POGGIANTI, B.
POMPEI, E.
Sadibekova, T.
VALTCHANOV, I.
MARULLI, F.
VEROPALUMBO, A.
Alis, Sinan
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Abstract
Context. Galaxy clusters trace the highest density peaks in the large-scale structure of the Universe. Their clustering provides a powerful probe that can be exploited in combination with cluster mass measurements to strengthen the cosmological constraints provided by cluster number counts.
URI
http://hdl.handle.net/20.500.12627/126665
https://doi.org/10.1051/0004-6361/201833238
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