Fig. 7
Spectral energy distribution for the new sources using the derived WMAP data and NED data of the possible counterparts. The arrows represent upper limits corresponding to 3σ, where σ was obtained from the pixel noise. The WMAP data are plotted with data from MRC 0427-539B and IC 2082 for Source # 1, PKS 0437-454 for Source # 2, PKS 0212-620 for Source # 3, PKS 0313-66019.0 for Source # 4 and PKS 0235-618 for Source # 5. For the Sources # 1, # 4, and # 5 , it is also plotted the BCES(Y | X) ordinary least-squares regression lines.
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