48 citations · 295 across the 12 of their papers we have counts for
12 papers
Galactic Foreground Constraints from the Python V Cosmic Microwave Background Anisotropy Data
Pia Mukherjee, Kim Coble, Mark Dragovan +4
We constrain Galactic foreground contamination of the Python V cosmic microwave background anisotropy data by cross correlating it with foreground contaminant emission templates. T…
CMB Anisotropy Constraints on Flat-Lambda and Open CDM Cosmogonies from DMR, UCSB South Pole, Python, ARGO, MAX, White Dish, OVRO, and SuZIE Data
Pia Mukherjee, Ken Ganga, Bharat Ratra +4
We use joint likelihood analyses of combinations of fifteen cosmic microwave background (CMB) anisotropy data sets from the DMR, UCSB South Pole 1994, Python I--III, ARGO, MAX 4 an…
Galactic Foregrounds in OVRO and UCSB South Pole 1994 Cosmic Microwave Background Anisotropy Data
Pia Mukherjee, Brian Dennison, Bharat Ratra +3
We study Galactic emission foreground contamination of the OVRO and UCSB South Pole 1994 cosmic microwave background (CMB) anisotropy data by cross-correlating with templates of in…
First Results from Viper: Detection of Small-Scale Anisotropy at 40 GHZ
J. B. Peterson, G. S. Griffin, M. G. Newcomb +7
Results of a search for small-scale anisotropy in the cosmic microwave background (CMB) are presented. Observations were made at the South Pole using the Viper telescope, with a .2…
Python I, II, and III CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
Graca Rocha, Radoslaw Stompor, Ken Ganga +4
We use Python I, II, and III cosmic microwave background anisotropy data to constrain cosmogonies. We account for the Python beamwidth and calibration uncertainties. We consider op…
ARGO CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
Bharat Ratra, Ken Ganga, Radoslaw Stompor +3
We use data from the ARGO cosmic microwave background (CMB) anisotropy experiment to constrain cosmogonies. We account for the ARGO beamwidth and calibration uncertainties, and mar…