Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background

Table 1

Full-sky foreground-cleaned CMB maps from WMAP data used in our analysis to estimate the variable 𝑦 (see the text for more details). Note that the reference [78] includes the analysis of maps from the three- and five-year WMAP releases.

Full sky maps	References
Hinshaw et al.	[14, 79]
de Oliveira-Costa et al.	[80]
Kim et al.	[78]
Park et al.	[81]
Delabrouille et al.	[82]