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Cosmic Microwave Background Anisotropy Measurement from Python V

  • Published:2003-02-20 Issue:2 Volume:584 Page:585-592
  • ISSN:0004-637X
  • Container-title:The Astrophysical Journal
  • language:en
  • Short-container-title:ApJ

Author:

Coble K.,Dodelson S.,Dragovan M.,Ganga K.,Knox L.,Kovac J.,Ratra B.,Souradeep T.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference27 articles.

Cited by 15 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

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2. On the road to percent accuracy: non-linear reaction of the matter power spectrum to dark energy and modified gravity;Monthly Notices of the Royal Astronomical Society;2019-07-04

3. How to optimally constrain galaxy assembly bias: supplement projected correlation functions with count-in-cells statistics;Monthly Notices of the Royal Astronomical Society;2019-06-25

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. EVOLUTION OF MASSIVE PROTOSTARS WITH HIGH ACCRETION RATES;The Astrophysical Journal;2009-01-19
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