Thomas, Peter - Department of Physics and Astronomy, University of Sussex

• Constructing the Universe with Clusters of Galaxies, IAP 2000 meeting, Paris (France) July 2000 Florence Durret & Daniel Gerbal eds.
• arXiv:astroph/9908107 Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 16 April 2000 (MN L A T E X style file v1.4)
• arXiv:1002.4539v1[astro-ph.CO]24Feb2010 Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 24 February 2010 (MN LATEX style file v2.2)
• Mon. Not. R. Astron. Soc. 000, 000--000 (2000) The Alignment of Clusters using Large Scale Simulations
• arXiv:astroph/9908062 Mon. Not. R. Astron. Soc. 000, 000--000 (1999) Printed 5 June 2000 (MN L A T E X style file v1.4)
• Mon. Not. R. Astron. Soc. 317, 3744 (2000) Hydrodynamical simulations of the SunyaevZel'dovich effect
• Mon. Not. R. Astron. Soc. 377, 317334 (2007) doi:10.1111/j.1365-2966.2007.11605.x The evolution of clusters in the CLEF cosmological simulation: X-ray
• DRAFT VERSION FEBRUARY 2, 2001 Preprint typeset using L A T E X style emulateapj v. 21/08/00
• SunyaevZel'dovich predictions for the Planck Surveyor satellite using the Hubble Volume simulations
• Mon. Not. R. Astron. Soc. 323, 743756 (2001) Multiphase smoothed-particle hydrodynamics
• Measuring the three-dimensional shear from simulation data, with applications to weak gravitational lensing
• arXiv:0910.0117v1[astro-ph.CO]1Oct2009 The role of active galactic nuclei in galaxy
• Mon. Not. R. Astron. Soc. 313, 229236 (2000) Peculiar velocities of galaxy clusters
• -Croton D. J., Springel V., White S.D.M., et.al., 2006, MNRAS, 365, 11-28 -De Lucia G. & Blaizot J., 2007, MNRAS, 375, 2-14
• Peter Thomas University of Sussex Merger simulations: equal mass, o -centre
• Simulations of galaxy clusters Peter Thomas -Astronomy Centre, University of Sussex
• Not. Astron. 209214 (2000) J. Colberg, D. M. White,
• Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 2 July 1997 (MN L A T E X style file v1.4) The structure of galaxy clusters in different cosmologies
• The Astrophysical Journal, 552:L27L30, 2001 May 1 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• arXiv:astroph/9907224 Preprint astroph/9907224
• The alignment of clusters using large-scale simulations Lesley I. Onuoraw
• Mon. Not. R. Astron. Soc. 348, 14011408 (2004) doi:10.1111/j.1365-2966.2004.07463.x Hydrodynamical simulations of the SunyaevZel'dovich effect
• arXiv:astroph/0007348 Mon. Not. R. Astron. Soc. 000, 1--14 (2000) Printed 24 July 2000 (MN L A T E X style file v1.4)
• GALAXY CLUSTERS HUBBLE VOLUME SIMULATIONS: COSMOLOGICAL CONSTRAINTS FROM SURVEY POPULATIONS
• Mon. Not. R. Astron. Soc. 348, 1401--1408 (2004) doi:10.1111/j.13652966.2004.07463.x Hydrodynamical simulations of the Sunyaev--Zel'dovich effect
• Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 10 October 1996 (MN L A T E X style file v1.3) Mass constraints from multiphase cooling flow models
• arXiv:astroph/9310024 An Owner's Guide to Smoothed Particle Hydrodynamics
• Mon. Not. R. Astron. Soc. 340, 12401248 (2003) The mass function of primordial star clusters
• Mon. Not. R. Astron. Soc. 396, 535547 (2009) doi:10.1111/j.1365-2966.2009.14730.x Monte Carlo Markov Chain parameter estimation in semi-analytic
• Mon. Not. R. Astron. Soc. 341, 12461252 (2003) Simulated X-ray cluster temperature maps
• Mon. Not. R. Astron. Soc. 000, 1--18 (2000) Printed 28 October 2000 (MN L A T E X style file v1.4) Simulations of galaxy formation in a cosmological volume
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• Mon. Not. R. Astron. Soc. 379, 11431154 (2007) doi:10.1111/j.1365-2966.2007.11997.x The recycling of gas and metals in galaxy formation: predictions of a
• Simulations of deep pencil-beam redshift surveys N. Yoshida,1P
• Mon. Astron. 1240--1248 (2003) The mass function primordial star clusters
• Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 21 February 1996 (MN L A T E X style file v1.3) Merger trees and the multiplicity function of halos
• Mon. Not. R. Astron. Soc. 319, 721727 (2000) In-shock cooling in numerical simulations
• arXiv:astroph/0002437 Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 6 April 2000 (MN L A T E X style file v1.4)
• Mon. Not. R. Astron. Soc. 000, 000{000 (0000) Printed 17 March 2003 (MN L A T E X style le v2.2) The impact of galaxy formation on X-ray groups
• arXiv:astroph/0102352 preprint astro-ph/0102352
• Preprint typeset using L A T E X style emulateapj v. 21/08/00 THE IMPACT OF COOLING AND HEATING ON THE SUNYAEV{ZEL'DOVICH EFFECT
• The Astrophysical Journal, 521:L99L102, 1999 August 20 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 22 February 1996 (MN L A T E X style file v1.3) The Baryon Catastrophe and the multiphase intracluster
• Parameter tests within cosmological simulations of galaxy formation Scott T. Kay,1w
• Mon. Not. R. Astron. Soc. 319, 267288 (2000) Weak gravitational lensing in different cosmologies, using an algorithm
• How big were the first cosmological objects? Roger M. Hutchings,1
• The Millennium Gas project aims to undertake smoothed-particle hydrodynamic resimulations of the Millennium Simulation, providing many hundred massive galaxy clusters for comparison with X-ray surveys (170 clusters with kTsl > 3 keV). This paper looks at
• Mon. Not. R. Astron. Soc. 000, 000{000 (0000) Printed 19 December 2001 (MN L A T E X style le v2.2) Can simulations reproduce the observed temperature{mass
• Cosmology using the Parkes Hi Multibeam SouthernSky Survey
• arXiv:0909.2150v1[astro-ph.CO]11Sep2009 Mon. Not. R. Astron. Soc. 000, 113 (2009) Printed 11 September 2009 (MN LATEX style file v2.2)
• arXiv:astro-ph/0411649v123Nov2004 F. Combes, D. Barret, T. Contini, F. Meynadier and L. Pagani (eds)
• arXiv:astroph/9903320 Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 7 March 2000 (MN L A T E X style file v1.4)
• Clusters of galaxies: new results from the CLEF hydrodynamics simulation
• THE ASTROPHYSICAL JOURNAL, 525:554582, 1999 November 10 The American Astronomical Society. All rights reserved. Printed in U.S.A.(1999.
• Mon. Not. R. Astron. Soc. 310, 453464 (1999) Weak gravitational lensing in the standard cold dark matter model, using
• Mon. Not. R. Astron. Soc. 317, 10291040 (2000) The effect of radiative cooling on the X-ray properties of galaxy clusters
• A simulated tCDM cosmology cluster catalogue: the NFW profile and the temperaturemass scaling relations
• Hydrodynamical simulations of the SunyaevZel'dovich effect: the kinetic effect
• Simulations of galaxy formation in a cosmological volume F. R. Pearce,1,2P
• The Astrophysical Journal, 561:L15L18, 2001 November 1 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Can simulations reproduce the observed temperaturemass relation for clusters of galaxies?
• Simulations of the formation, evolution and clustering of galaxies and quasars
• EVOLUTION OF X-RAY CLUSTER SCALING RELATIONS IN SIMULATIONS WITH RADIATIVE COOLING AND NONGRAVITATIONAL HEATING
• Mon. Not. R. Astron. Soc. 386, 20152021 (2008) doi:10.1111/j.1365-2966.2008.13127.x Nature versus nurture: the curved spine of the galaxy cluster X-ray
• Mon. Not. R. Astron. Soc. 386, 21102114 (2008) doi:10.1111/j.1365-2966.2008.13183.x The SunyaevZel'dovich temperature of the intracluster medium
• Mon. Not. R. Astron. Soc. 389, 102112 (2008) doi:10.1111/j.1365-2966.2008.13543.x Formation of ultra-compact dwarf galaxies: tests of the galaxy threshing
• The Astrophysical Journal, 704:915929, 2009 October 20 doi:10.1088/0004-637X/704/2/915 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• Mon. Not. R. Astron. Soc. 405, 375386 (2010) doi:10.1111/j.1365-2966.2010.16458.x Globular cluster formation within the Aquarius simulation
• Mon. Not. R. Astron. Soc. 383, 16491654 (2008) doi:10.1111/j.1365-2966.2007.12684.x The effect of dwarf galaxy disruption in semi-analytic models
• The physics of structure formation in the Universe Peter Thomas -Astronomy Centre, University of Sussex
• Mon. Not. R. Astron. Soc. 413, 691704 (2011) doi:10.1111/j.1365-2966.2010.18165.x Baryon fractions in clusters of galaxies: evidence against a pre-heating
• GALAXY CLUSTERS IN HUBBLE VOLUME SIMULATIONS: COSMOLOGICAL CONSTRAINTS FROM SKY SURVEY POPULATIONS
• Mon. Not. R. Astron. Soc. 375, 184190 (2007) doi:10.1111/j.1365-2966.2006.11282.x The orientation of galaxy dark matter haloes around cosmic voids
• Hydrodynamic simulations of merging clusters of galaxies Benedict W. Ritchie1,2P
• R. Astron. 336, 527--540 (2002) The effect cooling and preheating on the Xray properties of clusters
• Mon. Not. R. Astron. Soc. 000, 1{11 (2000) Printed 8 February 2001 (MN L A T E X style le v1.4) How big were the rst cosmological objects?
• astroph/9809221 Mon. Not. R. Astron. Soc. 000, 1--30 (1998) Printed 19 August 1999 (MN L A T E X style file v1.4)
• Peter Thomas University of Sussex Evolution of Cluster Scaling Relations
• arXiv:astroph/0011212 Mon. Not. R. Astron. Soc. 000, 1{8 (2000) Printed 13 November 2000 (MN L A T E X style le v1.4)
• arXiv:astroph/0310493 Preprint astro-ph/0310493
• Mon. Not. R. Astron. Soc. 319, 619648 (2000) Smoothed Particle Hydrodynamics in cosmology: a comparative study
• ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS**
• arXiv:astroph/0107374 Mon. Not. R. Astron. Soc. 000, 000{000 (0000) Printed 20 July 2001 (MN L A T E X style le v2.2)
• Hydra: AN ADAPTIVE--MESH IMPLEMENTATION OF P 3 M--SPH H.M.P. Couchman
• Peter Thomas University of Sussex Entropy Excess without Preheating
• Mon. Not. R. Astron. Soc. 336, 527540 (2002) The effect of cooling and preheating on the X-ray properties of clusters
• arXiv:astro-ph/0509803v127Sep2005 Draft version September 28, 2005
• R. Astron. 346, 319--326 (2003) The power spectrum amplitude from clusters revisited: using
• arXiv:astroph/0011187 Preprint astro-ph/0011187
• Mon. Not. R. Astron. Soc. 341, 1311--1332 (2003) Stable clustering, the halo model and nonlinear cosmological
• Preprint astro-ph/yymmnnn Baryon fractions in clusters of galaxies: evidence against a
• Mon. Not. R. Astron. Soc. 368, 13011310 (2006) doi:10.1111/j.1365-2966.2006.10222.x On the population of primordial star clusters in the presence of ultraviolet
• Mon. Not. R. Astron. Soc. 343, 608618 (2003) The impact of galaxy formation on X-ray groups
• Mon. Not. R. Astron. Soc. 399, 17731794 (2009) doi:10.1111/j.1365-2966.2009.15402.x Galaxiesintergalactic medium interaction calculation I. Galaxy
• Simulated cluster evolution Peter Thomas
• The Millennium Gas Simulations Peter Thomas
• Mon. Not. R. Astron. Soc. 000, 113 (2011) Printed 12 September 2011 (MN LATEX style file v2.2) Confronting theoretical models with the observed
• Mon. Not. R. Astron. Soc. 000, 127 (2005) Printed 20 January 2012 (MN LATEX style file v2.2) SunyaevZel'dovich clusters in Millennium Gas simulations
• Heating and enriching the intracluster medium C. J. Short1