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An international team of researchers, including Carnegie Mellon University’s Rachel Mandelbaum, has shown that the relationship between galaxy clusters and their surrounding dark matter halo is more c...
We measure the filling factor, correlation function, and power spectrum of transmitted flux in a large sample of Lyα forest spectra, comprised of 30 Keck HIRES spectra and 23 Keck LRIS spectra. We inf...
The clustering dipole of the local universe from the Two Micron All Sky Survey     galaxies  clusters       font style='font-size:12px;'> 2014/12/24
The unprecedented sky coverage and photometric uniformity of the Two Micron All Sky Survey (2MASS) provides a rich resource for investigating the galaxies populating the local universe. A full charact...
Galaxy clustering and galaxy bias in a Lambda CDM universe     formation  large-scale structure of universe       font style='font-size:12px;'> 2014/12/24
We investigate galaxy clustering and the correlations between galaxies and mass in the ΛCDM cosmological model (inflationary cold dark matter with Ωm = 0.4, ΩΛ = 0.6, h = 0.65, n = 0.95, and σ8 = 0.8)...
On the Clustering of Sub-millimeter Galaxies     correlation function  10-meter telescope       font style='font-size:12px;'> 2014/12/20
We measure the angular two-point correlation function of sub-millimeter galaxies (SMGs) from 1.1-millimeter imaging of the COSMOS field with the AzTEC camera and ASTE 10-meter telescope. These data yi...
Dark Matter Halos: Assembly, Clustering and Sub-halo Accretion     Dark matter  Galaxy formation  Halos       font style='font-size:12px;'> 2014/12/9
I carried out systematic studies on the assembly history of dark matter halos, using numerical simulations and semi-analytical methods. First, I look into dark halo mass assembly history. I confirmed ...
Evolution in the clustering strength of radio galaxies     galaxies  active  Galaxies  galaxies  evolution  Galaxies       font style='font-size:12px;'> 2011/10/20
We cross match the NVSS and FIRST surveys with three large photometric catalogues of luminous red galaxies (LRGs) to define radio-loud samples. These have median redshifts 0.35, 0.55 and 0.68 and, by ...
Large-scale clustering of galaxies in general relativity     Large-scale clustering  galaxies  general relativity       font style='font-size:12px;'> 2011/10/17
Several recent studies have shown how to properly calculate the observed clustering of galaxies in a relativistic context, and uncovered corrections to the Newtonian calculation that become significan...
We present a detailed investigation of the changing relationship between galaxies and the dark matter haloes they inhabit from z ~ 1.2 to the present day. We do this by comparing precise galaxy cluste...
Clustering in the Great Attractor Region     Clustering  Great Attractor Region       font style='font-size:12px;'> 2009/6/11
Clustering in the Great Attractor Region。
We inquire the phenomena of clustering of galaxies in an expanding universe from a theoretical point of view on the basis of thermodynamics and correlation functions. The partial differential equation...
We inquire the phenomena of clustering of galaxies in an expanding universe from a theoretical point of view on the basis of thermodynamics and correlation functions. The partial differential equation...

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