ON THE CLUSTER PHYSICS OF SUNYAEV–ZEL'DOVICH AND X-RAY SURVEYS. II. DECONSTRUCTING THE THERMAL SZ POWER SPECTRUM
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J. R. Bond | J. L. Sievers | J. Bond | N. Battaglia | C. Pfrommer | J. Sievers | C. Pfrommer | N. Battaglia | J. Bond
[1] Martin White,et al. Dark matter halo abundances, clustering and assembly histories at high redshift , 2007, 0706.0208.
[2] Y. Jing,et al. ACCURATE UNIVERSAL MODELS FOR THE MASS ACCRETION HISTORIES AND CONCENTRATIONS OF DARK MATTER HALOS , 2008, 0811.0828.
[3] A. Broderick,et al. THE COSMOLOGICAL IMPACT OF LUMINOUS TeV BLAZARS. III. IMPLICATIONS FOR GALAXY CLUSTERS AND THE FORMATION OF DWARF GALAXIES , 2011, 1106.5505.
[4] Power spectrum of the Sunyaev-Zel’dovich effect , 1999, astro-ph/9912180.
[5] J. Silk,et al. Cosmology and large scale structure , 1996 .
[6] J. Bond,et al. The Peak-Patch Picture of Cosmic Catalogs. I. Algorithms , 1996 .
[7] Jeremiah P. Ostriker,et al. SIMULATIONS OF THE MICROWAVE SKY , 2009, 0908.0540.
[8] R. B. Barreiro,et al. Planck early results - X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters , 2011, 1101.2043.
[9] M. White,et al. Hydrodynamic Simulations of the Sunyaev-Zeldovich Effect(s) , 2000, astro-ph/0008133.
[10] Concentrations of Dark Halos from Their Assembly Histories , 2001, astro-ph/0108151.
[11] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[12] M. Lueker,et al. A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE , 2011, 1105.3182.
[13] J. Huchra,et al. Groups of galaxies. I. Nearby groups , 1982 .
[14] Edward J. Wollack,et al. THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGICAL PARAMETERS FROM THE 2008 POWER SPECTRUM , 2010, 1009.0866.
[15] J. Bond,et al. Accepted for publication in The Astrophysical Journal Preprint typeset using L ATEX style emulateapj v. 11/26/04 , 2022 .
[16] Michael S. Warren,et al. Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality , 2008, 0803.2706.
[17] J. Bond,et al. The Kinetic Sunyaev-Zel'dovich Effect from Radiative Transfer Simulations of Patchy Reionization , 2007 .
[18] G. Efstathiou,et al. A Simple Empirically Motivated Template for the Unresolved Thermal Sunyaev-Zeldovich Effect , 2011, 1106.3208.
[19] J. Bond,et al. ON THE CLUSTER PHYSICS OF SUNYAEV–ZEL'DOVICH AND X-RAY SURVEYS. I. THE INFLUENCE OF FEEDBACK, NON-THERMAL PRESSURE, AND CLUSTER SHAPES ON Y–M SCALING RELATIONS , 2011, 1109.3709.
[20] Edward J. Wollack,et al. SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: POWER SPECTRA AND WMAP-DERIVED PARAMETERS , 2010, 1001.4635.
[21] Peter A. R. Ade,et al. THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM AT 148 AND 218 GHz FROM THE 2008 SOUTHERN SURVEY , 2010, 1009.0847.
[22] P. A. R. Ade,et al. IMPROVED CONSTRAINTS ON COSMIC MICROWAVE BACKGROUND SECONDARY ANISOTROPIES FROM THE COMPLETE 2008 SOUTH POLE TELESCOPE DATA , 2010, 1012.4788.
[23] Harvard,et al. Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium , 2007, astro-ph/0703661.
[24] S. More,et al. THE OVERDENSITY AND MASSES OF THE FRIENDS-OF-FRIENDS HALOS AND UNIVERSALITY OF HALO MASS FUNCTION , 2011, 1103.0005.
[25] D. Weinberg,et al. Cosmological Simulations with TreeSPH , 1995, astro-ph/9509107.
[26] The Sunyaev Zel'dovich effect: simulation and observation , 2002, astro-ph/0201375.
[27] J. Silk. COSMIC BLACK-BODY RADIATION AND GALAXY FORMATION. , 1968 .
[28] D. Weinberg,et al. The Effects of Gasdynamics, Cooling, Star Formation, and Numerical Resolution in Simulations of Cluster Formation , 1999, astro-ph/9907097.
[29] J. R. Bond,et al. Cosmological Results from Five Years of 30 GHz CMB Intensity Measurements with the Cosmic Background Imager , 2009, 0901.4540.
[30] S. Cole,et al. The structure of dark matter haloes in hierarchical clustering models , 1995, astro-ph/9510147.
[31] S. Kay,et al. Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology , 2008, 0804.2486.
[32] H. Trac,et al. TEMPLATES FOR THE SUNYAEV–ZEL’DOVICH ANGULAR POWER SPECTRUM , 2010, 1006.2828.
[33] J. Bond,et al. Current models of the observable consequences of cosmic reionization and their detectability , 2007, astro-ph/0702099.
[34] S. Cole,et al. Sunyaev–Zel'dovich fluctuations in the cold dark matter scenario , 1988 .
[35] Todd A. Thompson,et al. Radiation Pressure-supported Starburst Disks and Active Galactic Nucleus Fueling , 2005 .
[36] K. Dawson,et al. Final Results from the BIMA CMB Anisotropy Survey and Search for a Signature of the Sunyaev-Zel'dovich Effect , 2006, astro-ph/0602413.
[37] O. Zahn,et al. MODELING EXTRAGALACTIC FOREGROUNDS AND SECONDARIES FOR UNBIASED ESTIMATION OF COSMOLOGICAL PARAMETERS FROM PRIMARY COSMIC MICROWAVE BACKGROUND ANISOTROPY , 2011, 1102.5195.
[38] G. Bryan,et al. Statistical Properties of X-Ray Clusters: Analytic and Numerical Comparisons , 1997, astro-ph/9710107.
[39] Kenneth Levenberg. A METHOD FOR THE SOLUTION OF CERTAIN NON – LINEAR PROBLEMS IN LEAST SQUARES , 1944 .
[40] A. Lewis,et al. Cosmological parameters from CMB and other data: A Monte Carlo approach , 2002, astro-ph/0205436.
[41] A SIMPLE AND ACCURATE MODEL FOR INTRACLUSTER GAS , 2005, astro-ph/0504334.
[42] J. Carlstrom,et al. Understanding Cluster Gas Evolution and Fine-Scale Cosmic Microwave Background Anisotropy with Deep Sunyaev-Zeldovich Effect Surveys , 2001, astro-ph/0105229.
[43] D. Nagai,et al. IMPACT OF CLUSTER PHYSICS ON THE SUNYAEV–ZEL'DOVICH POWER SPECTRUM , 2010, 1006.1945.
[44] G. Voit. Tracing cosmic evolution with clusters of galaxies , 2004, astro-ph/0410173.
[45] O. Zahn,et al. SHARPENING THE PRECISION OF THE SUNYAEV–ZEL'DOVICH POWER SPECTRUM , 2009, 0903.5322.
[46] Deprojecting Sunyaev-Zeldovich Statistics , 2000, astro-ph/0007462.
[47] Nick Kaiser,et al. Evolution and clustering of rich clusters , 1986 .
[48] Michael S. Warren,et al. Precision Determination of the Mass Function of Dark Matter Halos , 2005, astro-ph/0506395.
[49] Uros Seljak,et al. The Sunyaev-Zel'dovich angular power spectrum as a probe of cosmological parameters , 2002 .
[50] H. M. P. Couchman,et al. The mass function of dark matter haloes , 2000, astro-ph/0005260.
[51] Hydrodynamical simulations of the Sunyaev-Zel'dovich effect , 1999, astro-ph/9907224.
[52] Y. Suto,et al. Anisotropies in the Microwave Background Due to the Sunyaev-Zel'dovich Effect from Virialized Objects at High Redshifts , 1993 .
[53] P. Madau,et al. Radiative Transfer in a Clumpy Universe. II. The Ultraviolet Extragalactic Background , 1995, astro-ph/9509093.
[54] J. Bond,et al. How filaments of galaxies are woven into the cosmic web , 1995, Nature.
[55] Matthias Bartelmann,et al. Detecting Sunyaev–Zel'dovich clusters with Planck – II. Foreground components and optimized filtering schemes , 2004, astro-ph/0407090.
[56] Detecting Sunyaev-Zel'dovich clusters with Planck - I. Construction of all-sky thermal and kinetic SZ maps , 2004, astro-ph/0407089.
[57] S. White,et al. A Universal Density Profile from Hierarchical Clustering , 1996, astro-ph/9611107.
[58] M. Donahue,et al. THE PRESSURE PROFILES OF HOT GAS IN LOCAL GALAXY GROUPS , 2010, 1012.0312.
[59] Non-Gaussian Aspects of Thermal and Kinetic Sunyaev-Zel'dovich Effects , 2001, astro-ph/0105063.
[60] E. Komatsu,et al. Universal gas density and temperature profile , 2001, astro-ph/0106151.
[61] J. M. Gelb,et al. Cosmological N‐Body Simulations , 1991 .
[62] Y. Zeldovich,et al. Small-scale fluctuations of relic radiation , 1970, Astrophysics and Space Science.
[63] G. Efstathiou,et al. The evolution of large-scale structure in a universe dominated by cold dark matter , 1985 .
[64] J. R. Bond,et al. SIMULATIONS OF THE SUNYAEV–ZEL'DOVICH POWER SPECTRUM WITH ACTIVE GALACTIC NUCLEUS FEEDBACK , 2010, 1003.4256.
[65] P. A. R. Ade,et al. HIGH-RESOLUTION CMB POWER SPECTRUM FROM THE COMPLETE ACBAR DATA SET , 2008, 0801.1491.
[66] G. W. Pratt,et al. The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y-SZ-M-500 relation , 2009, 0910.1234.
[67] R. B. Barreiro,et al. Planck early results Special feature Planck early results . XI . Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations , 2011 .
[68] The probability distribution function of the Sunyaev-Zel'dovich power spectrum: An analytical approach , 2007, astro-ph/0701879.
[69] D. Marquardt. An Algorithm for Least-Squares Estimation of Nonlinear Parameters , 1963 .
[70] V. Springel,et al. Cosmological smoothed particle hydrodynamics simulations: a hybrid multiphase model for star formation , 2002, astro-ph/0206393.
[71] G. W. Pratt,et al. Planck early results Special feature Planck early results . VIII . The all-sky early Sunyaev-Zeldovich cluster sample , 2011 .
[72] P. A. R. Ade,et al. THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE 600 < ℓ < 8000 COSMIC MICROWAVE BACKGROUND POWER SPECTRUM AT 148 GHz , 2010, 1001.2934.
[73] A. Szalay,et al. The statistics of peaks of Gaussian random fields , 1986 .
[74] E. Komatsu,et al. Sunyaev-Zeldovich Fluctuations from Spatial Correlations between Clusters of Galaxies , 1999, The Astrophysical journal.
[75] Adrian T. Lee,et al. CONSTRAINTS ON THE HIGH-ℓ POWER SPECTRUM OF MILLIMETER-WAVE ANISOTROPIES FROM APEX-SZ , 2009, 0904.3939.
[76] P. A. R. Ade,et al. MEASUREMENTS OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH THE SOUTH POLE TELESCOPE , 2009, 0912.4317.