The radio-source population at 95 GHz

Physics

Scientific paper

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Extragalactic, Atca

Scientific paper

Improving our knowledge of the radio-source population at 95 GHz is crucial for interpreting the data from next-generation CMB missions like Planck. Earlier results from this program have shown that the surface density of 95 GHz sources which make up the polarized foreground in Planck images is significantly lower (by almost a factor of two at 100 mJy) than predicted by extrapolation from the source populations seen in low-frequency surveys. We propose new 95 GHz follow-up observations of a sample of 200 faint AT20G sources in order to investigate the radio spectra, polarization properties and variability of the high-frequency source population in more detail.

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