Consistency between the radio and MIR faint source counts using the radio-MIR correlation
arXiv:astro-ph/0403240 · doi:10.1142/9789812702432_0040
Abstract
We show from the recent extrapolation of the radio-FIR correlation to the MIR that the 20 cm and 15 um differential source counts are likely to come from the same parent population.
2 pages, 2 figures, to appear in proceedings of 'Multi-wavelength AGN surveys', Cozumel, 2003