The evolution of assembly bias
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C. Baugh | I. Zehavi | N. Padilla | S. Contreras | I. Lacerna | Esteban Jim'enez | E. Jiménez | Nelson Padilla
[1] A. Robotham,et al. Shark: introducing an open source, free, and flexible semi-analytic model of galaxy formation , 2018, Monthly Notices of the Royal Astronomical Society.
[2] Manodeep Sinha,et al. Connecting and dissecting galaxies’ angular momenta and neutral gas in a hierarchical universe: cue Dark Sage , 2018, Monthly Notices of the Royal Astronomical Society.
[3] J. Tinker,et al. Halo histories versus galaxy properties at z = 0 II: large-scale galactic conformity , 2018 .
[4] P. Norberg,et al. The impact of assembly bias on the halo occupation in hydrodynamical simulations , 2018, Monthly Notices of the Royal Astronomical Society.
[5] Zheng Zheng,et al. Dependence of halo bias and kinematics on assembly variables , 2017, Monthly Notices of the Royal Astronomical Society.
[6] Durham,et al. The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5 , 2017, 1708.07628.
[7] C. Baugh,et al. The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos , 2017, 1706.07871.
[8] Yale,et al. The immitigable nature of assembly bias: the impact of halo definition on assembly bias , 2017, 1705.04327.
[9] R. Wechsler,et al. Beyond assembly bias: exploring secondary halo biases for cluster-size haloes , 2017, 1705.03888.
[10] V. Gonzalez-Perez,et al. Galactic conformity measured in semi-analytic models , 2017, 1703.10175.
[11] A. Hopkins,et al. A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups , 2017, 1703.06657.
[12] S. Lilly,et al. On the evidence for large-scale galactic conformity in the local Universe , 2017, 1702.08460.
[13] S. White,et al. Assembly bias and splashback in galaxy clusters , 2017, 1702.01682.
[14] N. Padmanabhan,et al. Halo assembly bias from Separate Universe simulations , 2016, 1612.02833.
[15] E. Rykoff,et al. On the Level of Cluster Assembly Bias in SDSS , 2016, 1611.00366.
[16] C. Baugh,et al. The evolution of the galaxy content of dark matter haloes , 2016, 1607.06154.
[17] Simon J. Mutch,et al. SEMI-ANALYTIC GALAXY EVOLUTION (SAGE): MODEL CALIBRATION AND BASIC RESULTS , 2016, 1601.04709.
[18] Erik Tollerud,et al. Introducing decorated HODs: modelling assembly bias in the galaxy–halo connection , 2015, 1512.03050.
[19] Qi Guo,et al. Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models , 2015, 1512.00015.
[20] Perth,et al. A unified multiwavelength model of galaxy formation , 2015, 1509.08473.
[21] R. Mandelbaum,et al. Mapping stellar content to dark matter haloes – II. Halo mass is the main driver of galaxy quenching , 2015, 1509.06758.
[22] Andrew P. Hearin,et al. Connecting massive galaxies to dark matter haloes in BOSS - I. Is galaxy colour a stochastic process in high-mass haloes? , 2015, 1509.00482.
[23] J. Schaye,et al. Subhalo abundance matching and assembly bias in the EAGLE simulation , 2015, 1507.01948.
[24] V. Springel,et al. An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations , 2015, 1507.01942.
[25] Zheng Zheng,et al. Accurate and efficient halo-based galaxy clustering modelling with simulations , 2015, 1506.07523.
[26] S. More,et al. Evidence of Halo Assembly Bias in Massive Clusters. , 2015, Physical review letters.
[27] Andrew P. Hearin,et al. Assessing Colour-dependent Occupation Statistics Inferred from Galaxy Group Catalogues , 2015, 1505.04798.
[28] R. Mandelbaum,et al. ON DETECTING HALO ASSEMBLY BIAS WITH GALAXY POPULATIONS , 2015, 1504.07632.
[29] C. Conselice,et al. Tracing galaxy populations through cosmic time: a critical test of methods for connecting the same galaxies between different redshifts at z < 3 , 2015, 1504.05583.
[30] C. Baugh,et al. The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass? , 2015, 1502.06614.
[31] S. White,et al. Galaxy formation in the Planck cosmology – I. Matching the observed evolution of star formation rates, colours and stellar masses , 2014, 1410.0365.
[32] Andrew P. Hearin,et al. Beyond halo mass: galactic conformity as a smoking gun of central galaxy assembly bias , 2014, 1404.6524.
[33] Carlton M. Baugh,et al. How sensitive are predicted galaxy luminosities to the choice of stellar population synthesis model , 2013, 1309.7057.
[34] W. Percival,et al. The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the low-redshift sample , 2014, 1401.4171.
[35] S. Cole,et al. N-body dark matter haloes with simple hierarchical histories , 2013, 1311.6649.
[36] Andrew P. Hearin,et al. Galaxy assembly bias: a significant source of systematic error in the galaxy–halo relationship , 2013, 1311.1818.
[37] B. Andrews,et al. EXPLORING THE CHEMICAL LINK BETWEEN LOCAL ELLIPTICALS AND THEIR HIGH-REDSHIFT PROGENITORS , 2013, 1310.7020.
[38] G. Lucia,et al. Detection of galaxy assembly bias , 2013, 1305.0350.
[39] C. Baugh,et al. How robust are predictions of galaxy clustering , 2013, 1301.3497.
[40] S. White,et al. Simulations of the galaxy population constrained by observations from z = 3 to the present day: implications for galactic winds and the fate of their ejecta , 2012, 1212.1717.
[41] N. Padilla,et al. The nature of assembly bias – II. Halo spin , 2012, 1207.4476.
[42] C. Baugh,et al. The clustering of Hα emitters at z = 2.23 from HiZELS , 2012 .
[43] S. White,et al. Galaxy formation in WMAP1 and WMAP7 cosmologies , 2012, 1206.0052.
[44] N. Padilla,et al. The nature of assembly bias – III. Observational properties , 2011, 1110.6174.
[45] Y. Mellier,et al. Galaxy clustering in the CFHTLS-Wide: the changing relationship between galaxies and haloes since z ~ 1.2 , 2011, 1107.0616.
[46] N. Padilla,et al. The nature of assembly bias – I. Clues from a ΛCDM cosmology , 2010, 1011.1498.
[47] A. Benson. Galacticus: A Semi-Analytic Model of Galaxy Formation , 2010, 1008.1786.
[48] Santiago,et al. Clustering and descendants of MUSYC galaxies at z < 1.5 , 2010, 1006.5645.
[49] Andrew J. Benson,et al. Galaxy formation theory , 2010, 1006.5394.
[50] G. Kauffmann,et al. Erratum: From dwarf spheroidals to cD galaxies: simulating the galaxy population in a ΛCDM cosmology , 2010, 1006.0106.
[51] R. Nichol,et al. GALAXY CLUSTERING IN THE COMPLETED SDSS REDSHIFT SURVEY: THE DEPENDENCE ON COLOR AND LUMINOSITY , 2010, 1005.2413.
[52] Britton D. Smith,et al. HOW WELL DO COSMOLOGICAL SIMULATIONS REPRODUCE INDIVIDUAL HALO PROPERTIES? , 2010, 1001.5037.
[53] J. Newman,et al. Galaxy assembly bias on the red sequence , 2009, 0910.0245.
[54] Durham,et al. The clustering of Lyα emitters in a ΛCDM Universe , 2008, 0807.3447.
[55] C. Lagos,et al. Effects of AGN feedback on ΛCDM galaxies , 2008, 0805.1930.
[56] Zheng Zheng,et al. Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering , 2007, 0712.3570.
[57] P. Norberg,et al. Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment? , 2007, 0707.3445.
[58] P. Thomas,et al. The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model , 2007, astro-ph/0701407.
[59] S. White,et al. Assembly bias in the clustering of dark matter haloes , 2006, astro-ph/0611921.
[60] Y. Suto,et al. The Dependence of Dark Halo Clustering on Formation Epoch and Concentration Parameter , 2006, astro-ph/0610099.
[61] C. Baugh,et al. A primer on hierarchical galaxy formation: the semi-analytical approach , 2006, astro-ph/0610031.
[62] M. Blanton,et al. What Aspects of Galaxy Environment Matter? , 2006, astro-ph/0608353.
[63] G. Lucia,et al. The hierarchical formation of the brightest cluster galaxies , 2006, astro-ph/0606519.
[64] S. White,et al. Halo assembly bias and its effects on galaxy clustering , 2006, astro-ph/0605636.
[65] Ravi K. Sheth U. Pittsburgh,et al. The environmental dependence of galaxy clustering in the Sloan Digital Sky Survey , 2006, astro-ph/0601407.
[66] J. Frieman,et al. Percolation Galaxy Groups and Clusters in the SDSS Redshift Survey: Identification, Catalogs, and the Multiplicity Function , 2006, astro-ph/0601346.
[67] Zheng Zheng,et al. The Dependence of the Occupation of Galaxies on the Halo Formation Time , 2006, astro-ph/0601120.
[68] Oxford,et al. Breaking the hierarchy of galaxy formation , 2005, astro-ph/0511338.
[69] G. Kauffmann,et al. The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colour , 2005, astro-ph/0508046.
[70] S. White,et al. The age dependence of halo clustering , 2005, astro-ph/0506510.
[71] J. Peacock,et al. Simulations of the formation, evolution and clustering of galaxies and quasars , 2005, Nature.
[72] H. Mo,et al. Galaxy occupation statistics of dark matter haloes: observational results , 2004, astro-ph/0410114.
[73] J. Frieman,et al. The Luminosity and Color Dependence of the Galaxy Correlation Function , 2004, astro-ph/0408569.
[74] R. Davé,et al. Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies , 2004, astro-ph/0408564.
[75] S. White,et al. The subhalo populations of ΛCDM dark haloes , 2004, astro-ph/0404589.
[76] Padova,et al. On the environmental dependence of halo formation , 2004, astro-ph/0402237.
[77] Simon D. M. White,et al. Chemical enrichment of the intracluster and intergalactic medium in a hierarchical galaxy formation model , 2003, astro-ph/0310268.
[78] Potsdam,et al. The Dark Side of the Halo Occupation Distribution , 2003, astro-ph/0308519.
[79] C. Baugh,et al. The Halo Occupation Distribution and the Physics of Galaxy Formation , 2002, astro-ph/0212357.
[80] R. Sheth,et al. Halo Models of Large Scale Structure , 2002, astro-ph/0206508.
[81] D. Weinberg,et al. The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and Mass , 2001, astro-ph/0109001.
[82] Padova,et al. Populating a cluster of galaxies - I. Results at z=0 , 2000, astro-ph/0012055.
[83] A. Dekel,et al. A Universal Angular Momentum Profile for Galactic Halos , 2000, astro-ph/0011001.
[84] J. Peacock,et al. Halo occupation numbers and galaxy bias , 2000, astro-ph/0005010.
[85] G. Kauffmann,et al. Clustering of galaxies in a hierarchical universe - I. Methods and results at z=0 , 1998, astro-ph/9805283.
[86] G. Kauffmann,et al. Environmental influences on dark matter haloes and consequences for the galaxies within them , 1997, astro-ph/9710125.
[87] S. White,et al. The Structure of cold dark matter halos , 1995, astro-ph/9508025.
[88] C. Frenk,et al. A recipe for galaxy formation , 1994, astro-ph/9402001.
[89] S. Cole,et al. Merger rates in hierarchical models of galaxy formation – II. Comparison with N-body simulations , 1994, astro-ph/9402069.
[90] S. D. M. White,et al. The merging history of dark matter haloes in a hierarchical universe , 1993 .
[91] J. R. Bond,et al. Excursion set mass functions for hierarchical Gaussian fluctuations , 1991 .
[92] G. Efstathiou,et al. The evolution of large-scale structure in a universe dominated by cold dark matter , 1985 .
[93] M. Rees,et al. Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering , 1978 .
[94] William H. Press,et al. Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation , 1974 .
[95] U. Chicago,et al. The Astrophysical Journal, in press Preprint typeset using L ATEX style emulateapj v. 6/22/04 THE DEPENDENCE OF HALO CLUSTERING ON HALO FORMATION HISTORY, CONCENTRATION, AND OCCUPATION , 2005 .