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The 1% Concordance Hubble Constant

, , , и . (2014)cite arxiv:1406.1718Comment: 25 pages, 4 figures, submitted to the Astrophysical Journal.

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Clemens L J Engel

Walter L J Rosen

Ute L J Pröschel

Clemens L J Engel

J L M Wagenvoort

 

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Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, , , , , , , , , и 11 other автор(ы). (2010)cite arxiv:1001.4538 Comment: 57 pages, 20 figures. Accepted for publication in ApJS. (v2) References added. The SZ section expanded with more analysis. The discrepancy between the KS and X-ray derived profiles has been resolved. (v3) New analysis of the SZ effect on individual clusters added (Section 7.3). The LCDM parameters have been updated using the latest recombination history code (RECFAST version 1.5).The 1% Concordance Hubble Constant, , , и . (2014)cite arxiv:1406.1718Comment: 25 pages, 4 figures, submitted to the Astrophysical Journal.First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters, , , , , , , , , и 7 other автор(ы). (июня 2003)Beyond optical depth: Future determination of ionization history from the CMB, , , и . (2019)cite arxiv:1910.00590Comment: 12 pages, 10 figures, submitted to ApJ.Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, , , , , , , , , и 9 other автор(ы). (2008)cite arxiv:0803.0547 Comment: 52 pages, 21 figures, accepted for publication in ApJS. (v2) References added. Cosmological parameters updated with the latest union supernova compilation (Kowalski et al. arXiv:0804.4142).