“…developed techniques to account for uncertainties, such as those in the beamwidth and calibration, in likelihood analyses of cosmic microwave background (CMB) anisotropy data. GRGS and Ganga et al (1997bGanga et al ( ,1998 used these techniques, in conjunction with theoretical CMB anisotropy spectra, in analyses of the UCSB South Pole 1994 (Gundersen et al 1995), the SuZIE (Church et al 1997), and the MAX 4+5 (Tanaka et al 1996;Lim et al 1996, and references therein) CMB anisotropy data sets. Bond & Jaffe (1997) have also analyzed the UCSB South Pole 1994 data and the Saskatoon (Netterfield et al 1997) data.…”