Consistency between the radio and MIR faint source counts using the radio-MIR correlation
Astrophysics
2017-08-23 v1
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.
Cite
@article{arxiv.astro-ph/0403240,
title = {Consistency between the radio and MIR faint source counts using the radio-MIR correlation},
author = {N. Seymour and I. M. McHardy and K. Gunn},
journal= {arXiv preprint arXiv:astro-ph/0403240},
year = {2017}
}
Comments
2 pages, 2 figures, to appear in proceedings of 'Multi-wavelength AGN surveys', Cozumel, 2003