ACT Data Products at LAMBDA
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Likelihood software
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This is the software used by the ACT collaboration to compute the likelihood of cosmological models, using the small-scale microwave power spectrum measured by ACT from the 2008 Southern sky survey. It is based on the WMAP team's likelihood software.
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1 file 4.6 mb |
TAR BALL
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Beams
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The beam window functions for the ACT temperature power spectra are computed at 148 GHz and 218 GHz. They are obtained by transforming the beam profiles obtained from Saturn observations.
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2 file 451 kb each |
ASCII
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Spectra
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The ACT temperature power spectra are computed at 148 GHz and 218 GHz. Three spectra are given, for 148x148, 148x218, and 218x218.
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3 file 4 kb each |
ASCII
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Source Templates
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The angular power spectra shape due to clustered IR point sources as predicted by two different models (named Src-1, Src-2) are supplied for the 148 GHZ ACT frequency.
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2 file 221 kb each |
ASCII
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SZ Templates
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The angular power spectra due to the Sunyaev-Zeldovich effect as predicted by four different models (named TBO-1, TBO-2, Battaglia, Shaw) are supplied for the 148 GHZ ACT frequency.
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6 file < 557 kb each |
ASCII
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SZ Clusters 2008 Data
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Catalog of 23 galaxy clusters detected by the Sunyaev-Zel'dovich (SZ)
effect in 455 square degrees of sky surveyed by ACT during 2008 at 148
GHz. The catalog gives the cluster names, positions, redshifts,
signal-to-noise, and measured SZ signal. SZ and optical images of each
cluster are also included.
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N/A |
TAR BALL
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Point Source Catalog
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This is a catalog of 157 point sources detected in a 148 GHz data collected by ACT during its 2008 observing season.
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1 file 20 kb |
ASCII
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Back To Suborbital CMB Experiment Page
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