66 citations · 250 across the 14 of their papers we have counts for
14 papers
The ATESP 5 GHz radio survey IV. 19, 38, and 94 GHz observations and radio spectral energy distributions
R. Ricci, I. Prandoni, H. R. De Ruiter +1
It is now established that the faint radio population is a mixture of star-forming galaxies and faint active galactic nuclei (AGNs), with the former dominating below S(1.4GHz) \sim…
Molecular Disks in Radio Galaxies: The pathway to ALMA
I. Prandoni, R. A. Laing, H. R. de Ruiter +1
Context. It has recently been proposed that the jets of low-luminosity radio galaxies are powered by direct accretion of the hot phase of the IGM onto the central black hole. Cold…
The ATESP 5 GHz radio survey. III. 4.8, 8.6 and 19 GHz follow-up observations of radio galaxies
I. Prandoni, H. R. de Ruiter, R. Ricci +3
[Abridged] Physical and evolutionary properties of the sub-mJy radio population are not entirely known. The radio/optical analysis of the ATESP 5 GHz sample has revealed a signific…
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…
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…
A Molecular Gas Study of Low Luminosity Radio Galaxies
I. Prandoni, R. A. Laing, P. Parma +3
We discuss CO spectral line data of a volume-limited sample of 23 nearby (z<0.03) low luminosity radio galaxies, selected from the B2 catalogue. We investigate whether the CO prope…