Anisotropy of the Microwave Sky at 90 GHz: Results from Python II
Astrophysics
2009-10-28 v1
Abstract
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 Python instrument yielded a statistically significant sky signal; in this paper we report the confirmation of that signal with data taken in the second year, and on results from an interleaving set of fields.
Cite
@article{arxiv.astro-ph/9508065,
title = {Anisotropy of the Microwave Sky at 90 GHz: Results from Python II},
author = {J. E. Ruhl and M. Dragovan and S. R. Platt and J. Kovac and G. Novak},
journal= {arXiv preprint arXiv:astro-ph/9508065},
year = {2009}
}
Comments
10 pages, plus 2 figures. Postscript and uufiles versions available via anonymous ftp at ftp://astro.uchicago.edu/pub/astro/ruhl/pyII