Fig. 22.
Comparison of BeeP’s Free flux densities at 353 GHz (upper row) and 545 GHz (lower row) with aperture flux-density values (APERFLUX) from PCCS2+2E. The blue contours ([68, 95, 99]%) show the distribution of the PCCS2 subset of sources and the red ones the remaining PCCS2E. Unlike in Fig. 20, BeeP sources whose position shifted by more than one pixel from the original PCCS2+2E and those with EXT ≥ 1.64 pixels (extended) are not included.
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