An essential input to SZ experimental simulations are simulated Compton y maps of the sky together with corresponding cluster catalogs. I currently have 3 nice sets of LCDM simulations:
Here are a few plots comparing these three:
Comparing the catalogs: Note that WHS and Bia agree pretty well, whereas SW has approx twice as many clusters of given mass.
Comparing the y maps: The WHS maps have more small scale power.
Here are the first three actual maps with color scale truncated at y=3e-5. Click here for all of them.