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

MARULLI, F.; VEROPALUMBO, A.; SERENO, M.; MOSCARDINI, L.; PACAUD, F.; Pierre, M.; PLIONIS, M.; CAPPI, A.; ADAMI, C.; Alis, SİNAN; ALTIERI, B.; Birkinshaw, M.; ETTORI, S.; Faccioli, L.; GASTALDELLO, F.; Koulouridis, E.; LIDMAN, C.; LE FEVRE, J.; MAUROGORDATO, S.; POGGIANTI, B.; POMPEI, E.; Sadibekova, T.; VALTCHANOV, I.

doi:10.1051/0004-6361/201833238

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

MARULLI F., VEROPALUMBO A., SERENO M., MOSCARDINI L., PACAUD F., Pierre M., ...Daha Fazla

ASTRONOMY & ASTROPHYSICS, cilt.620, 2018 (SCI-Expanded, Scopus)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 620
Basım Tarihi: 2018
Doi Numarası: 10.1051/0004-6361/201833238
Dergi Adı: ASTRONOMY & ASTROPHYSICS
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Anahtar Kelimeler: X-rays: galaxies: clusters, cosmology: observations, large-scale structure of Universe, cosmological parameters, BARYON ACOUSTIC-OSCILLATIONS, SPATIAL CORRELATION-FUNCTION, POWER SPECTRUM, RICH CLUSTERS, COSMOLOGICAL MODELS, DARK ENERGY, SKY SURVEY, CONSTRAINTS, BIAS, CALIBRATION
İstanbul Üniversitesi Adresli: Evet

Özet

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.