Spectrum of the Anomalous Microwave Emission in the North Celestial Pole with WMAP 7-Year Data

Figure 5

Colored lines: likelihoods for 𝑛_H for different values of 𝑇 as detailed in the legend; black line: likelihood for 𝑛_H marginalized over 𝑇. (a) 𝑥_H=0.001, 𝜒=1; (b) same as (a) with 𝜒=0.1; (c, d): same as (a) with 𝑥_H=0.01 (c) and 𝑥_H=0.1 (d).

(a)

(b)

(c)

(d)