作者: C. G. Bornancini , N. D. Padilla , D. G. Lambas , C. De Breuck
DOI: 10.1111/J.1365-2966.2006.10120.X
关键词: Radio galaxy 、 Galaxy group 、 Physics 、 Elliptical galaxy 、 Astronomy 、 Galaxy 、 Astrophysics 、 Luminous infrared galaxy 、 Galaxy cluster 、 Quasar 、 Galaxy formation and evolution
摘要: We present measurements of the clustering properties galaxies in field redshift range 0.5 ≤ z 1.5 Ultra Steep Spectrum radio sources selected from Sydney University Molonglo Sky Survey and National Radio Astronomy Observatories Very Large Array Survey. Galaxies these USS fields were identified deep near-infrared observations, complete down to K s = 20, using IRIS2 instrument at Anglo-Australian Telescope. used distribution < 20 taken Cimatti et al. (2002) constrain correlation length r 0 . find a strong signal with around our sample. A comoving 14.0 ± 2.8 h -1 Mpc y 1.98 0.15 are derived flat cosmological model universe. compare findings those obtained N-body simulation populated GALFORM semi-analytic galaxies. that clusters masses M 10 13.4-14.2 2 ⊙ have cluster-galaxy cross-correlation amplitude comparable found between hosts These results suggest distant excellent tracers galaxy overdensities pinpoint progenitors day rich