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We develop a Maximum Likelihood estimator (MLE) to measure the masses of galaxy clusters through the impact of gravitational lensing on the temperature and polarization anisotropies of the cosmic microwave background (CMB).
1916
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1945
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Sunyaev R. and Zel’dovich Ya. B., Small-Scale Fluctuations of Relic Radiation
1970
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Sunyaev R. and Zel’dovich Ya. B., The velocity of clusters of galaxies relative to the microwave background - The possibility of its measurement
1980
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Einasto J. and Haud U., Galactic models with massive corona. I - Method. II - Galaxy
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Kamionkowski M., Kosowsky A. and Stebbins A., Statistics of cosmic microwave background polarization
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Sazonov S. Y. and Sunyaev R. A., Microwave polarization in the direction of galaxy clusters induced by the CMB quadrupole anisotropy
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Seljak U., and Zaldarriaga M., Lensing Induced Cluster Signatures in Cosmic Microwave Background
2000
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Seljak U., Analytic model for galaxy and dark matter clustering
2000
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Lewis A., Challinor A., and Lasenby A., HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere
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King L. and Schneider P., Cluster mass profiles from weak lensing II
2001
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Cooray A., and Sheth R., Halo Models of Large Scale Structure
2002
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Carlstrom J. E., Holder G. P., and Reese E. D., Cosmology with the Sunyaev-Zel’dovich Effect
2002
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Dodelson S., CMB-cluster lensing
2004
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Holder G. and Kosowsky A., Gravitational Lensing of the Microwave Background by Galaxy Clusters
2004
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Maturi M., Bartelmann M., Meneghetti M., Moscardini L., Gravitational lensing of the CMB by galaxy clusters
2005
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2005
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de Zotti G., Ricci R., Mesa D. et al., Predictions for high-frequency radio surveys of extragalactic sources
2005
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González-Nuevo J., Toffolatti L., and Argüeso F., Predictions of the Angular Power Spectrum of Clustered Extragalactic Point Sources at Cosmic Microwave Background Frequencies from Flat and All-Sky Two-dimensional Simulations
2005
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Lewis A. and King L., Cluster masses from CMB and galaxy weak lensing
2006
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Hartlap J., Simon P., Schneider P., Why your model parameter confidences might be too optimistic. Unbiased estimation of the inverse covariance matrix
2006
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Hu W., DeDeo S., and Vale C., Cluster mass estimators from CMB temperature and polarization lensing
2007
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2007
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Seiffert M, Borys C., Scott D, Halpern M., An upper limit to polarized submillimetre emission in Arp 220
2007
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2008
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Cardoso J., Le Jeune M., Delabrouille J., Betoule M., Patanchon G., Component Separation With Flexible Models?Application to Multichannel Astrophysical Observations
2008
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Baumann D., Jackson M. G., Adshead P. et al., Probing Inflation with CMB Polarization
2014
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2014
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2014
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Planck Collaboration XII, Planck 2013 results. XII. Diffuse component separation
2014
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2009
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Refregier A., Amara A., Kitching T. D. et al., Euclid Imaging Consortium Science Book
2010
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2010
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2010
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2011
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2011
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2011
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2012
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2015
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2015
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Melin J. and Bartlett J., Measuring cluster masses with CMB lensing: a statistical approach
2015
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Madhavacheril M. et al., Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos
2015
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2015
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2016
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2016
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Abazajian N. K., Adshead P., Ahmed Z. et al., CMB-S4 Science Book, First Edition
2016
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2016
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2016
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Battaglia N., The Tau of Galaxy Clusters
2016
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2016
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Suzuki A. Ade P. A. R, Akiba Y. et al., The Polarbear-2 and the Simons Array Experiments
2016
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Planck Collaboration XIII, Planck 2015 results. XIII. Cosmological parameters
2016
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2016
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