STACKED WEAK LENSING MASS CALIBRATION: ESTIMATORS, SYSTEMATICS, AND IMPACT ON COSMOLOGICAL PARAMETER CONSTRAINTS
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[1] Cheng Li,et al. Three Different Types of Galaxy Alignment within Dark Matter Halos , 2007, 0704.0674.
[2] E. Rozo,et al. Size bias in galaxy surveys. , 2009, Physical review letters.
[3] Michael S. Warren,et al. Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality , 2008, 0803.2706.
[4] J. Frieman,et al. CONSTRAINING THE SCATTER IN THE MASS–RICHNESS RELATION OF maxBCG CLUSTERS WITH WEAK LENSING AND X-RAY DATA , 2008, 0809.2794.
[5] Stacking Weak-Lensing Signals of Sunyaev-Zel'dovich Clusters to Constrain Cluster Physics , 2006, astro-ph/0601254.
[6] E. Rozo,et al. WEAK-LENSING PEAK FINDING: ESTIMATORS, FILTERS, AND BIASES , 2010, 1009.0757.
[7] J. Frieman,et al. COSMOLOGICAL CONSTRAINTS FROM THE SLOAN DIGITAL SKY SURVEY MaxBCG CLUSTER CATALOG , 2009, 0902.3702.
[8] E. Rozo,et al. LENSING BIAS IN COSMIC SHEAR , 2009, 0904.4703.
[9] Martin White,et al. Cluster galaxy dynamics and the effects of large-scale environment , 2010, 1005.3022.
[10] Risa H. Wechsler,et al. ANNEALING A FOLLOW-UP PROGRAM: IMPROVEMENT OF THE DARK ENERGY FIGURE OF MERIT FOR OPTICAL GALAXY CLUSTER SURVEYS , 2009, 0907.2690.
[11] Jiangang Hao,et al. IMPROVEMENT OF THE RICHNESS ESTIMATES OF maxBCG CLUSTERS , 2009 .
[12] Subhabrata Majumdar,et al. Importance of Cluster Structural Evolution in Using X-Ray and Sunyaev-Zeldovich Effect Galaxy Cluster Surveys to Study Dark Energy , 2002 .
[13] Carlos Cunha,et al. Cross-calibration of cluster mass-observables , 2008, 0812.0583.
[14] A. Hornstrup,et al. CHANDRA CLUSTER COSMOLOGY PROJECT. II. SAMPLES AND X-RAY DATA REDUCTION , 2008, 0805.2207.
[15] J. Peacock,et al. Stable clustering, the halo model and non-linear cosmological power spectra , 2002, astro-ph/0207664.
[16] H. Hoekstra,et al. THE X-RAY CLUSTER NORMALIZATION OF THE MATTER POWER SPECTRUM , 2008, 0809.3832.
[17] R. Mandelbaum,et al. A halo mass—concentration relation from weak lensing , 2008, 0805.2552.
[18] Alexey Vikhlinin,et al. Cluster constraints on f (R) gravity , 2009, 0908.2457.
[19] Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution , 2005, astro-ph/0503363.
[20] Masamune Oguri,et al. Combining cluster observables and stacked weak lensing to probe dark energy: Self-calibration of systematic uncertainties , 2010, 1010.0744.
[21] Michigan.,et al. Testable dark energy predictions from current data , 2009, 0912.3816.
[22] D. Nagai,et al. Submitted to the Astrophysical Journal Preprint typeset using L ATEX style emulateapj v. 11/12/01 RESPONSE OF DARK MATTER HALOS TO CONDENSATION OF BARYONS: COSMOLOGICAL SIMULATIONS AND IMPROVED ADIABATIC CONTRACTION MODEL , 2004 .
[23] J. Barentine,et al. A MaxBCG catalog of 13,823 galaxy clusters from the Sloan Digital Sky Survey , 2007 .
[24] H. Hoekstra. How well can we determine cluster mass profiles from weak lensing , 2002, astro-ph/0208351.
[25] Using Weak-Lensing Dilution to Improve Measurements of the Luminous and Dark Matter in A1689 , 2006, astro-ph/0608499.
[26] Self-calibration of cluster dark energy studies: Counts in cells , 2004, astro-ph/0401559.
[27] A. Lewis,et al. Efficient computation of CMB anisotropies in closed FRW models , 1999, astro-ph/9911177.
[28] Candace Oaxaca WrightTereasa G. Brainerd,et al. Gravitational Lensing by NFW Halos , 1999, astro-ph/9908213.
[29] Y. Mellier,et al. A WEAK LENSING STUDY OF X-RAY GROUPS IN THE COSMOS SURVEY: FORM AND EVOLUTION OF THE MASS–LUMINOSITY RELATION , 2009, 0910.5219.
[30] Subhabrata Majumdar,et al. Self-Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum, and Mass Measurements , 2003, astro-ph/0305341.
[31] P. Hall,et al. Cosmological Constraints from the Red-Sequence Cluster Survey , 2006, astro-ph/0603588.
[32] S. J. Lilly,et al. Precision photometric redshift calibration for galaxy–galaxy weak lensing , 2007, 0709.1692.
[33] Cosmological Constraints from the SDSS maxBCG Cluster Catalog , 2009 .
[34] J. Frieman,et al. CROSS-CORRELATION WEAK LENSING OF SDSS GALAXY CLUSTERS. I. MEASUREMENTS , 2007, 0709.1153.
[35] Likelihood methods for cluster dark energy surveys , 2006, astro-ph/0602147.
[36] Cross-correlation lensing: Determining galaxy and cluster mass profiles from statistical weak lensing measurements , 2005, astro-ph/0507467.
[37] S. White,et al. The Structure of cold dark matter halos , 1995, astro-ph/9508025.
[38] J. Frieman,et al. Constraining dark energy with clusters: Complementarity with other probes , 2009, 0904.1589.
[39] Stanford,et al. The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys , 2008, 0803.1491.
[40] L. Samushia,et al. Will multiple probes of dark energy find modified gravity , 2010, 1004.4810.
[41] Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy , 2006, astro-ph/0608681.
[42] S. W. Allen,et al. New constraints on dark energy from the observed growth of the most X-ray luminous galaxy clusters , 2007, 0709.4294.
[43] Michael R. Blanton,et al. Systematic errors in weak lensing: application to SDSS galaxy-galaxy weak lensing , 2005 .