Cosmic Microwave Background Anisotropy Measurement From Python V
We analyze observations of the microwave sky made with the Python experiment in its fifth year of operation at the Amundsen-Scott South Pole Station in Antarctica. After modeling the noise and constructing a map, we extract the cosmic signal from the data. We simultaneously estimate the angular powe...
Main Authors: | , , , , , , , |
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Format: | Text |
Language: | unknown |
Published: |
arXiv
2001
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Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0112506 https://arxiv.org/abs/astro-ph/0112506 |