A marked correlation function analysis of halo formation times in the Millennium Simulation
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S. Cole | C. Frenk | A. Jenkins | J. Helly | G. Harker
[1] G. Kauffmann,et al. The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colour , 2005, astro-ph/0508046.
[2] R. Sheth. The halo‐model description of marked statistics , 2005, astro-ph/0511772.
[3] S. White,et al. The age dependence of halo clustering , 2005, astro-ph/0506510.
[4] J. Peacock,et al. Simulations of the formation, evolution and clustering of galaxies and quasars , 2005, Nature.
[5] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[6] C. Baugh,et al. Where are the stars , 2004, astro-ph/0412049.
[7] J. Frieman,et al. Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey , 2004, astro-ph/0408003.
[8] Padova,et al. On the environmental dependence of halo formation , 2004, astro-ph/0402237.
[9] R. Nichol,et al. Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS , 2003, astro-ph/0311379.
[10] Rien van de Weygaert,et al. A hierarchy of voids: much ado about nothing , 2003, astro-ph/0311260.
[11] H. Mo,et al. The dependence of the galaxy luminosity function on large-scale environment , 2003, astro-ph/0310147.
[12] Stefan Gottloeber,et al. The structure of voids , 2003, astro-ph/0305393.
[13] C. Baugh,et al. The Halo Occupation Distribution and the Physics of Galaxy Formation , 2002, astro-ph/0212357.
[14] Christopher J. Miller,et al. Galaxy Star Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey , 2002, astro-ph/0210193.
[15] C. Baugh,et al. Galaxy formation using halo merger histories taken from N‐body simulations , 2002, astro-ph/0210141.
[16] M. Kerscher,et al. Correlations in the orientations of galaxy clusters , 2002, astro-ph/0209029.
[17] R. Sheth,et al. Halo Models of Large Scale Structure , 2002, astro-ph/0206508.
[18] Nmsu,et al. Spatial distribution of galactic halos and their merger histories , 2002, astro-ph/0203148.
[19] C. Baugh,et al. A comparison of gas dynamics in smooth particle hydrodynamics and semi-analytic models of galaxy formation , 2002, astro-ph/0202485.
[20] D. Weinberg,et al. The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and Mass , 2001, astro-ph/0109001.
[21] V. Springel,et al. GADGET: a code for collisionless and gasdynamical cosmological simulations , 2000, astro-ph/0003162.
[22] H. Mo,et al. Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes , 1999, astro-ph/9907024.
[23] Padova,et al. Populating a cluster of galaxies - I. Results at z=0 , 2000, astro-ph/0012055.
[24] C. Baugh,et al. Hierarchical galaxy formation , 2000, astro-ph/0007281.
[25] M. Kerscher,et al. Luminosity- and Morphology-dependent Clustering of Galaxies , 2000, astro-ph/0003358.
[26] U. Seljak. Analytic model for galaxy and dark matter clustering , 2000, astro-ph/0001493.
[27] S. White,et al. The structure and clustering of Lyman-break galaxies , 1998, astro-ph/9807341.
[28] G. Kauffmann,et al. Clustering of galaxies in a hierarchical universe - I. Methods and results at z=0 , 1998, astro-ph/9805283.
[29] U. California,et al. Semi-analytic modelling of galaxy formation: The local Universe , 1998, astro-ph/9802268.
[30] G. Kauffmann,et al. Environmental influences on dark matter haloes and consequences for the galaxies within them , 1997, astro-ph/9710125.
[31] H. M. P. Couchman,et al. Evolution of Structure in Cold Dark Matter Universes , 1997, astro-ph/9709010.
[32] U. Seljak,et al. A Line of sight integration approach to cosmic microwave background anisotropies , 1996, astro-ph/9603033.
[33] C. Frenk,et al. A recipe for galaxy formation , 1994, astro-ph/9402001.
[34] G. Kauffmann,et al. The formation and evolution of galaxies within merging dark matter haloes , 1993 .
[35] S. Cole,et al. Merger rates in hierarchical models of galaxy formation – II. Comparison with N-body simulations , 1994, astro-ph/9402069.
[36] J. R. Bond,et al. Excursion set mass functions for hierarchical Gaussian fluctuations , 1991 .
[37] R. Bower. The evolution of groups of galaxies in the Press-Schechter formalism , 1991 .
[38] S. Cole,et al. Biased clustering in the cold dark matter cosmogony , 1989 .
[39] G. Efstathiou,et al. The formation of dark halos in a universe dominated by cold dark matter , 1988 .
[40] A. Szalay,et al. The statistics of peaks of Gaussian random fields , 1986 .
[41] G. Efstathiou,et al. The evolution of large-scale structure in a universe dominated by cold dark matter , 1985 .
[42] M. Postman,et al. The morphology-density relation - The group connection , 1984 .
[43] A. Dressler. Galaxy morphology in rich clusters: Implications for the formation and evolution of galaxies , 1980 .
[44] M. Rees,et al. Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering , 1978 .