...v. 26/01/00 COSMOLOGICAL IMPLICATIONS OF THE BIMA 30 GHZ...
Thus, we conclude that the non–detections are to be expected in a low M universe, given the sensitivity and solid angle of the deepest SZE survey to date.doi:10.1086/344749YEN-TING LINDepartment of AstronomyJOSEPH J. MOHRThe Astrophysical journal...