This is the software used by the ACT collaboration to compute the likelihood of cosmological models, using the small-scale CMB power spectrum from
500 < l <3500 measured by ACT, derived from the 3-year data (2008-2010 observations). More...
This is the software used by the ACT collaboration to compute the multi-frequency likelihood of cosmological models, using the small-scale microwave power spectra measured by ACT from 500 < l < 10000 from the 3-year data (2008-2010 observations). More...
A single tarball is supplied, containing the lensing likelihood and data for ACT. It is a simple chisq routine that takes in a theoretical deflection spectrum, and compares it to the ACT data file in the /data directory. More...
The ACT temperature power spectra are computed at 148 GHz and 218 GHz. Three spectra are given for each region (ACT-E and ACT-S), for 148x148, 148x218, and 218x218. The coadded spectra are also given. More...
The ACT temperature power spectra are combined to estimated the CMB bandpowers, marginalized over foregrounds and SZ. Spectra are given for each region (ACT-E and ACT-S). More...
2 files, < 3 KB each
ASCII
Data release products for South 2008 data at 148 GHz
These files contain the Atacama Cosmology Telescope (ACT) temperature maps of the southern stripe field, observed
during the 2008 season, in the 148 GHz band, and produced for the first ACT data release in March 2012. More...
These files contain combined hit-count maps for each pixel of Atacama Cosmology Telescope (ACT) maps of the southern stripe field, observed during the 2008 season, in the 148 GHz band, and produced for the first ACT data
release in March 2012. More...
These two files represent the radial beam profile and the Fourier
space window function of the ACT beam, appropriate for use with the
ACT 148 GHz maps of 2008 data released with Dunner et al. More...
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 likelihood software. More...
These are MCMC chains run using the ACT likelihood software based on the small-scale microwave power spectrum measured from the 2008 Southern sky survey. More...
This is the software and chains used by the ACT collaboration in Hlozek et al 2011 [1105.4887]. It includes the modification to CAMB required to use a binned primordial power spectrum instead of a power law, and modifications to CosmoMC to sample these additional parameters. More...
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. More...
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. More...
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. More...
This tarball includes 6 chains run for the lcdm+curvature model, with results reported in Sherwin et al 2011 (astro-ph/1103.0419), using WM
AP 7-year data plus ACT lensing likelihood described in Das et al 2011 (astro-ph/1103.2124). More...
Catalog of 23 galaxy clusters detected by the Sunyaev-Zeldovich (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.