Sunyaev-Zel'dovich Effect and secondary CMB anisotropy

SZE detections and images are now robust. The next step is to do large scale blind surveys - these (hopefully) will be done in the next few years. Arcminute anisotropy is possibly on the verge of detection, but will need ALMA like sensitivity for its characterization. The next step - just in time for ALMA - will require detailed observations (i.e., high resolution WITH high brightness sensitivity). See next pages on SZE etc.