High Resolution Microwave Full Sky Simulations
Overview
Here are realistic, full-sky, half-arcminute resolution simulations of the microwave sky matched to the most recent astrophysical
observations. The primary purpose of these simulations is to test the data reduction pipeline for the Atacama Cosmology Telescope (ACT)
experiment; however, the frequency coverage has been widened beyond the ACT bands and the maps utilize the easily accessible HEALPix
format to make these simulations applicable to other current and near future microwave background experiments.
Some of the
novel features of these simulations are that the radio and infrared galaxy populations are correlated with the galaxy cluster and group
populations, the primordial microwave background is lensed by the dark matter structure in the simulation via a ray-tracing code, the
contribution to the thermal and kinetic Sunyaev-Zel'dovich (SZ) signals from galaxy clusters, groups, and the intergalactic medium has
been included, and the gas prescription to model the SZ signals has been refined to match the most recent X-ray observations.
The cosmology adopted in these simulations is also consistent with the WMAP 5-year parameter measurements. These simulations should
serve as a useful tool for microwave surveys to cross-check SZ cluster detection, power spectrum, and cross-correlation analyses.
For a full discussion see Sehgal et al. (2009).
Any questions may be sent to sehgal@slac.standford.edu
Please note that these links point directly at binary files; you should right click on the links and select
the "Save link as" option.
Each green dot represents a single map for the corresponding data type/frequency pair; each map is 3GB in size.
The blue squares point to compressed tarballs containing all
the maps in the corresponding column or row; the blue dot in the lower right corner points to a tarball containing all the maps.
More information...