HIGHLIGHTS
- who: MNRAS et al. from the Institute of Geophysics, The Czech Academy of Sciences, Bočnı́ II, Praha, Czech Republic have published the paper: Missing dust signature in the cosmic microwave background, in the Journal: (JOURNAL)
SUMMARY
Distortions of the CMB due to this C interaction comprise the μ-type (at z 105 ) and y-type (at z 104 ) distortions related to the photon-electron interactions, distortions produced by the reionized IGM and the presence of galactic and extragalactic foregrounds (Wright 1981; Chluba and amp; Sunyaev 2012; De Zotti et_al 2016). The foreground contamination . . .
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