Anisotropy in the Microwave Sky at 90 GH[CLC]z[/CLC]: Results from Python II | Zendy

J. E. Ruhl | Zendy; M. Dragovan | Zendy; Stephen R. Platt | Zendy; J. M. Kovac | Zendy; Giles Novak | Zendy

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Anisotropy in the Microwave Sky at 90 GH[CLC]z[/CLC]: Results from Python II

Author(s) -

J. E. Ruhl,

M. Dragovan,

Stephen R. Platt,

J. M. Kovac,

Giles Novak

Publication year - 1995

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/309739

Subject(s) - autocorrelation , amplitude , python (programming language) , sky , anisotropy , physics , gaussian , mathematics , interleaving , statistics , optics , astrophysics , computer science , quantum mechanics , operating system

We report on additional observations of degree scale anisotropy at 90~GHzfrom the Amundsen-Scott South Pole Station in Antarctica. Observations duringthe first season with the Python instrument yielded a statistically significantsky signal; in this paper we report the confirmation of that signal with datataken in the second year, and on results from an interleaving set of fields.Comment: 10 pages, plus 2 figures. Postscript and uufiles versions available via anonymous ftp at ftp://astro.uchicago.edu/pub/astro/ruhl/pyI

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