The XXL Survey II. The bright cluster sample: catalogue and luminosity function

Yazar
Ponman, T. J.
CHIAPPETTI, L.
Democles, J.
ECKERT, D.
EVRARD, A. E.
FACCIOLI, L.
GASTALDELLO, F.
GUENNOU, L.
Horellou, C.
TUFFS, R.
PACAUD, F.
CLERC, N.
Giles, P. A.
ADAMI, C.
SADIBEKOVA, T.
PIERRE, M.
Maughan, B. J.
Lieu, M.
LE FEVRE, J. P.
Smith, G. P.
VALAGEAS, P.
VALTCHANOV, I.
Willis, J. P.
Ziparo, F.
Alis, Sinan
IOVINO, A.
KOULOURIDIS, E.
LE BRUN, V.
LIDMAN, C.
Liske, J.
MAUROGORDATO, S.
MENANTEAU, F.
OWERS, M.
POGGIANTI, B.
POMAREDE, D.
POMPEI, E.
Rapetti, D.
REIPRICH, T. H.
ALTIERI, B.
ARDILA, F.
Baldry, I.
BENOIST, C.
Birkinshaw, M.
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Özet
Context. The XXL Survey is the largest survey carried out by the XMM-Newton satellite and covers a total area of 50 square degrees distributed over two fields. It primarily aims at investigating the large-scale structures of the Universe using the distribution of galaxy clusters and active galactic nuclei as tracers of the matter distribution. The survey will ultimately uncover several hundreds of galaxy clusters out to a redshift of similar to 2 at a sensitivity of similar to 10 (14) erg s (1) cm (2) in the [0.5-2] keV band.
Bağlantı
http://hdl.handle.net/20.500.12627/107730
https://doi.org/10.1051/0004-6361/201526891
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