... One of arxiv/astro-ph preprints, arxiv/0706.1703v1 discusses correlation between galactic HI and the cosmic microwavebackground (CMB) and reports no statistically significant correlation. ...
... MNRAS, 349, 1267 (2004): Predictions on the high-frequency polarization properties of extragalactic radio sources and implications for polarization measurements of the cosmic microwavebackground (Tucci et al.) . ...
... Bayesian methods have also been employed to quantify the uncertainty in the large-scale structure of the universe (Jasche & Wandelt 2013) and in secondary anisotropies of the cosmic microwavebackground radiation (Bull et al. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/etc/SvDKS2015_ApJ813_66_LIRA_pval.pdf -- 964.8 Кб -- 30.10.2015 Похожие документы
... One of arxiv/astro-ph preprints, arxiv/0706.1703v1 discusses correlation between galactic HI and the cosmic microwavebackground (CMB) and reports no statistically significant correlation. ...
... Jiashun Jin, Purdue University, 10/11/2005 14 ' Cosmic MicrowaveBackground (CMB) $ CMB: · Oldest light in the universe, a direct link to early universe · A relic of radiation when the universe 380, 000 years old · An almost perfect black body at a ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/jjs_20051011.pdf -- 1900.9 Кб -- 12.10.2005 Похожие документы
... errors in the inferred model parameters.9 In many subfields (exceptions include, e.g., gravi9 tational wave astrophysics, VIRGO Collaboration 2011, LIGO Collaboration 2010, and references therein; cosmic microwavebackground (CMB) analyses, Mather et al ...
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Ссылки http://hea-www.harvard.edu/AstroStat/astro193/Lee+2011_apj_731_2_126.pdf -- 2913.9 Кб -- 28.01.2015 Похожие документы
... Simulations show that Constellation-X data alone can obtain uncertainties on w to ±0.05 and, in combination with the microwavebackground data, constraints on w and its evolution that are substantially smaller. ...
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Ссылки http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf -- 258.4 Кб -- 28.06.2011 Похожие документы
... particles impinging on gas clouds (Bremmstrahlung and Pion decay); and a broader, smoother comp onent due to these energetic particles "b oosting" the energy of photons from the ubiquitous low energy (microwave and infrared) background (Inverse Compton ...