Issue |
A&A
Volume 447, Number 2, February IV 2006
|
|
---|---|---|
Page(s) | 405 - 412 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361:20053395 | |
Published online | 07 February 2006 |
Point source confusion in SZ cluster surveys
1
APC, 11 pl. Marcelin Berthelot, 75231 Paris Cedex 05, France (UMR 7164 CNRS, Université Paris 7, CEA, Observatoire de Paris) e-mail: bartlett@cdf.in2p3.fr
2
Department of Physics, University of California Davis, One Shields Avenue, Davis, CA , 95616 USA e-mail: melin@bubba.physics.ucdavis.edu
Received:
10
May
2005
Accepted:
20
September
2005
We examine the effect of point source confusion on
cluster detection in Sunyaev-Zel'dovich (SZ) surveys. A filter
matched to the spatial and spectral characteristics of the SZ signal optimally extracts clusters from the astrophysical
backgrounds. We
calculate the expected confusion (point source and primary cosmic
microwave background [CMB]) noise through this
filter and quantify its effect on the detection threshold for both
single and multiple frequency surveys. Extrapolating current radio
counts, we estimate that confusion from sources
below ~Jy limits single-frequency surveys to
detection thresholds of
10-6 arcmin2 at
30 GHz and
arcmin2 at 15 GHz (for
unresolved clusters in a 2 arcmin beam);
these numbers are highly uncertain, and an
extrapolation with flatter counts leads to much lower confusion limits.
Bolometer surveys must contend with an important population of
infrared point sources. We find that a three-band matched
filter with 1 arcmin resolution (in each band)
efficiently reduces confusion, but does not eliminate it:
residual point source and CMB fluctuations contribute significantly
to the total filter noise. In this light, we find that a 3-band
filter with a low-frequency channel (e.g, 90+150+220 GHz) extracts
clusters more effectively than one with a high frequency channel (e.g,
150+220+300 GHz).
Key words: cosmic microwave background / galaxies: clusters: general / methods: observational
© ESO, 2006
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