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Deutsche Physikalische Gessellschaft IOP Institute of Physics

Cluster mass estimators from CMB temperature and polarization lensing

Focus on Gravitational Lensing

Wayne Hu1,3, Simon DeDeo1 and Chris Vale2

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[1]
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Hu W 2001 Mapping the dark matter with the CMB damping tail Astrophys. J. Lett. 557 L79
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Hu W and Okamoto T 2002 Mass reconstruction with CMB polarization Astrophys. J. 574 566
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Johnston D E et al 2007 Cross-correlation lensing: determining galaxy and cluster mass profiles from statistical weak lensing measurements Astrophys. J. 656 27-41
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Amblard A, Vale C and White M 2004 Weak lensing of the CMB by large-scale structure New Astron. 9 687-704
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Hu W 2001 The angular trispectrum of the CMB Phys. Rev. D 64 083005
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Challinor A and Chon G 2002 Geometry of weak lensing of CMB polarization Phys. Rev. D 66 127301
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Okamoto T and Hu W 2003 CMB lensing reconstruction on the full sky Phys. Rev. D 67 083002
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Navarro J F, Frenk C S and White S D M 1997 A universal density profile from hiearchical lustering Astrophys. J. 490 493
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[20]
Vale C and Hu W 2007 in preparation

[21]
Bartelmann M 1996 Arcs from a universal dark-matter halo profile Astron. Astrophys. 313 697-702

[22]
Bullock J S et al 2001 Profiles of dark halos: evolution, scatter and environment Mon. Not. R. Astron. Soc. 321 559
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Lima M and Hu W 2005 Self-calibration of cluster dark energy studies: observable-mass distribution Phys. Rev. D 72 043006
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