most citedThe ATESP 5 GHz radio survey. II. Physical properties of the faint radio population

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astro-ph2008

A view of the sub-mJy populations, modelling and perspectives for future deep surveys

I. Prandoni, P. Parma, A. Mignano +5

We use deep multi-colour (UBVRIJK) images mostly taken in the framework of the ESO Deep Public Survey (DPS) to optically identify and derive photometric redshifts for a complete sa…

astro-ph20071 cited

The ATESP 5 GHz radio survey. II. Physical properties of the faint radio population

A. Mignano, I. Prandoni, L. Gregorini +5

One of the most debated issues about sub-mJy radio sources, which are responsible for the steepening of the 1.4 GHz source counts, is the origin of their radio emission. Particular…

astro-ph200666 cited

The ATESP 5 GHz radio survey I. Source counts and spectral index properties of the faint radio population

I. Prandoni, P. Parma, M. H. Wieringa +5

[Abridged] The nature and evolutionary properties of the faint radio population, responsible for the steepening observed in the 1.4 GHz source counts below 1 milliJy, are not yet e…

astro-ph200611 cited

ESO Imaging survey: Optical Deep Public Survey

A. Mignano, J. M. Miralles, L. da Costa +7

This paper presents new five passbands (UBVRI) optical wide-field imaging data accumulated as part of the DEEP Public Survey (DPS) carried out as a public survey by the ESO Imaging…

astro-ph200617 cited

ESO Imaging Survey: Infrared Deep Public Survey

L. F. Olsen, J. -M. Miralles, L. da Costa +8

This paper presents new J and Ks data obtained from observations conducted at the ESO 3.5m New Technology Telescope using the SOFI camera. These data were taken as part of the ESO…