Issue |
A&A
Volume 436, Number 1, June II 2005
|
|
---|---|---|
Page(s) | 37 - 46 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361:20041785 | |
Published online | 20 May 2005 |
Gravitational lensing of the CMB by galaxy clusters
1
Dipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 2, 35122 Padova, Italy e-mail: maturi@pd.astro.it
2
Institut für Theoretische Astrophysik, Universität Heidelberg, Albert-Ueberle Strasse 2, 69121 Heidelberg, Germany
3
Max-Planck-Institut für Astrophysik, PO Box 1317, 85740 Garching, Germany
4
Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
Received:
3
August
2004
Accepted:
24
February
2005
We adapt a non-linear filter proposed by Hu (2001) for detecting
lensing of the CMB by large-scale structures to recover
surface-density profiles of galaxy clusters from their localised,
weak gravitational lensing effect on CMB fields. Shifting the
band-pass of the filter to smaller scales, and normalising it such
as to reproduce the convergence rather than the deflection angle, we
find that the mean density profile of a sample of 100 clusters can
be recovered to better than 10% from well within the scale radius
to almost the virial radius. The kinetic Sunyaev-Zel'dovich effect
is shown to be a negligible source of error. We test the filter
applying it to data simulated using the characteristics of the
Atacama Cosmology Telescope (ACT), showing that it will be
possible to recover mean cluster profiles outside a radius of
corresponding to ACT's angular resolution.
Key words: cosmology: theory / galaxies: clusters: general / cosmic microwave background / gravitational lensing
© ESO, 2005
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