Galactic Foreground Constraints from the Python V Cosmic Microwave Background Anisotropy Data-Reference-Cited by-同舟云学术

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Galactic Foreground Constraints from the Python V Cosmic Microwave Background Anisotropy Data

Published:2003-08 Issue:2 Volume:592 Page:692-698
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Mukherjee Pia,Coble Kim,Dragovan Mark,Ganga Ken,Kovac John,Ratra Bharat,Souradeep Tarun

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/592/i=2/a=692/pdf

Reference52 articles.

1. Cosmological constraints from Archeops

2. Cosmic Microwave Background Anisotropy Measurement from Python V

3. Anisotropy in the Cosmic Microwave Background at Degree Angular Scales: Python V Results

4. Galactic Microwave Emission at Degree Angular Scales

5. Cross-Correlation of Tenerife Data with Galactic Templates—Evidence for Spinning Dust?

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1. The State-of-Play of Anomalous Microwave Emission (AME) research;New Astronomy Reviews;2018-02

2. EVIDENCE FOR ANOMALOUS DUST-CORRELATED EMISSION AT 8 GHz;The Astrophysical Journal;2012-04-04

3. Observations of the Polarisation of the Anomalous Microwave Emission: A Review;Advances in Astronomy;2012

4. Cosmic microwave background power spectrum estimation with non-circular beam and incomplete sky coverage;Monthly Notices of the Royal Astronomical Society;2009-04-11

5. The Beginning and Evolution of the Universe;Publications of the Astronomical Society of the Pacific;2008-03

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