Sachs–Wolfe effect

Results: 13



#Item
1arXiv:astro-ph/9508126v2  16 Jul 2009

arXiv:astro-ph/9508126v2 16 Jul 2009

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Source URL: background.uchicago.edu

Language: English - Date: 2015-01-06 12:05:33
2Outline • Angular Diameter Distance Location of peaks Degeneracy

Outline • Angular Diameter Distance Location of peaks Degeneracy

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Source URL: background.uchicago.edu

Language: English - Date: 2009-10-01 12:32:28
3Astronomy & Astrophysics A&A 557, L1DOI:

Astronomy & Astrophysics A&A 557, L1DOI:

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Source URL: www.aanda.org

Language: English
4New Cosmic Microwave Background measurements with the Degree Angular Scale Interferometer (DASI) at the Amundsen-Scott South Pole Station John Carlstrom, University of Chicago  Center for Astrophysical Research

New Cosmic Microwave Background measurements with the Degree Angular Scale Interferometer (DASI) at the Amundsen-Scott South Pole Station John Carlstrom, University of Chicago Center for Astrophysical Research

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Source URL: astro.uchicago.edu

Language: English - Date: 2001-05-22 13:49:33
5Can we avoid dark energy? James P. Zibin,∗ Adam Moss,† and Douglas Scott‡ Department of Physics & Astronomy, University of British Columbia, Vancouver, BC, V6T 1Z1 Canada (Dated: August 7, [removed]arXiv:0809.3761v2

Can we avoid dark energy? James P. Zibin,∗ Adam Moss,† and Douglas Scott‡ Department of Physics & Astronomy, University of British Columbia, Vancouver, BC, V6T 1Z1 Canada (Dated: August 7, [removed]arXiv:0809.3761v2

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Source URL: xxx.lanl.gov

Language: English - Date: 2011-08-07 04:33:49
627. Cosmic microwave background[removed]COSMIC MICROWAVE BACKGROUND Revised September 2013 by D. Scott (University of British Columbia) and G.F. Smoot (UCB/LBNL). Appendix A, describing the BICEP2 B-mode polarization resu

27. Cosmic microwave background[removed]COSMIC MICROWAVE BACKGROUND Revised September 2013 by D. Scott (University of British Columbia) and G.F. Smoot (UCB/LBNL). Appendix A, describing the BICEP2 B-mode polarization resu

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Source URL: pdg.lbl.gov

Language: English - Date: 2014-08-21 16:38:31
7Probing primordial non-Gaussianity via iSW measurements with SKA continuum surveys Alvise Raccanelli1,2 , Olivier Dor´e1,2 , David J. Bacon3 , Roy Maartens3,4 , Mario G. Santos4,5,6 , Stefano Camera6 , Tamara Davis7,8 ,

Probing primordial non-Gaussianity via iSW measurements with SKA continuum surveys Alvise Raccanelli1,2 , Olivier Dor´e1,2 , David J. Bacon3 , Roy Maartens3,4 , Mario G. Santos4,5,6 , Stefano Camera6 , Tamara Davis7,8 ,

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Source URL: authors.library.caltech.edu

Language: English - Date: 2014-12-22 17:26:09
825. Cosmic microwave background[removed]COSMIC MICROWAVE BACKGROUND Revised August 2011 by D. Scott (University of British Columbia) and G.F. Smoot (UCB/LBNL).

25. Cosmic microwave background[removed]COSMIC MICROWAVE BACKGROUND Revised August 2011 by D. Scott (University of British Columbia) and G.F. Smoot (UCB/LBNL).

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Source URL: pdg.lbl.gov

Language: English - Date: 2012-06-18 19:19:53
926. Cosmic microwave background[removed]COSMIC MICROWAVE BACKGROUND

26. Cosmic microwave background[removed]COSMIC MICROWAVE BACKGROUND

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Source URL: pdg.lbl.gov

Language: English - Date: 2013-12-18 14:58:58
10

PDF Document

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Source URL: arxiv.org

Language: English - Date: 2010-11-11 20:09:18