4 papers
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…
Anisotropy in the Cosmic Microwave Background at Degree Angular Scales: Python V Results
K. Coble, M. Dragovan, J. Kovac +12
Observations of the microwave sky using the Python telescope in its fifth season of operation at the Amundsen-Scott South Pole Station in Antarctica are presented. The system consi…
Anisotropy in the Microwave Sky at 90 GHz: Results From Python III
S. R. Platt, J. Kovac, M. Dragovan +2
The third year of observations with the Python microwave background experiment densely sample a region of sky that includes the fields measured during the first…
Anisotropy of the Microwave Sky at 90 GHz: Results from Python II
J. E. Ruhl, M. Dragovan, S. R. Platt +2
We report on additional observations of degree scale anisotropy at 90~GHz from the Amundsen-Scott South Pole Station in Antarctica. Observations during the first season with the Py…