activity
19972016
most citedA Decade of SN1993J: Discovery of Wavelength Effects in the Expansion Rate

87 citations · 620 across the 36 of their papers we have counts for

collaborators

36 papers

astro-ph.IM2016

RadioNet3 Study Group White Paper on: The Future Organisation and Coordination of Radio Astronomy in Europe

M. A. Garrett, P. Charlot, S. T. Garrington +8

The QueSERA Study Group (QSG) have been tasked by the RadioNet Board to produce a White Paper on the future organisation and coordination of radio astronomy in Europe. This White P…

astro-ph.GA2015★ 6 cited

A sample of weak blazars at milli-arcsecond resolution

F. Mantovani, M. Bondi, K. -H. Mack +3

We started a follow-up investigation of the Deep X-ray Radio Blazar Survey objects with declination >-10 deg. We undertook a survey with the EVN at 5GHz to make the first images of…

astro-ph.IM2014★ 23 cited

Very Long Baseline Interferometry with the SKA

Zsolt Paragi, Leith Godfrey, Cormac Reynolds +79

Adding VLBI capability to the SKA arrays will greatly broaden the science of the SKA, and is feasible within the current specifications. SKA-VLBI can be initially implemented by pr…

astro-ph.CO2013★ 5 cited

A 20 GHz Bright Sample for Delta > 72 deg - II. Multi-frequency Follow-up

R. Ricci, S. Righini, R. Verma +10

We present follow-up observations at 5, 8 and 30 GHz of the K-band Northern Wide Survey (KNoWS) 20 GHz Bright Sample, performed with the 32-m Medicina Radio Telescope and the 32-m…

astro-ph.CO2013★ 10 cited

Radio polarimetry of compact steep spectrum sources at sub-arcsecond resolution

F. Mantovani, A. Rossetti, W. Junor +2

Aims - We report new Very Large Array polarimetric observations of Compact Steep-Spectrum (CSS) sources at 8.4, 15, and 23GHz. Methods - Using multi-frequency VLA observations we h…

astro-ph.IM2013★ 31 cited

VLBI imaging throughout the primary beam using accurate UV shifting

John S. Morgan, F. Mantovani, A. T. Deller +5

For Very Long Baseline Interferometry (VLBI), the fringe spacing is extremely narrow compared to the field of view imposed by the primary beam of each element. This means that an e…