activity
19972019
most citedThe fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees

322 citations · 326 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2019★ 322 cited

The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees

K. Kuijken, C. Heymans, A. Dvornik +20

The Kilo-Degree Survey (KiDS) is an ongoing optical wide-field imaging survey with the OmegaCAM camera at the VLT Survey Telescope, specifically designed for measuring weak gravita…

astro-ph2008

Cold gas & mergers: fundamental difference in HI properties of different types of radio galaxies?

Bjorn Emonts, Raffaella Morganti, Tom Oosterloo +1

We present results of a study of large-scale neutral hydrogen (HI) gas in nearby radio galaxies. We find that the early-type host galaxies of different types of radio sources (comp…

astro-ph2004★ 1 cited

Fast Outflows of Neutral Hydrogen in Radio Galaxies

T. A. Oosterloo, R. Morganti, B. H. C. Emonts +1

AGN activity is known to drive fast outflows of gas. We report the discovery of fast outflows of neutral gas with velocities over 1000 km/s in a number of radio galaxies. In the be…

astro-ph2003

Tidal Remnants and Intergalactic HII Regions

T. Oosterloo, R. Morganti, E. M. Sadler +3

We report the discovery of two small intergalactic HII regions in the loose group of galaxies around the field elliptical NGC 1490. The HII regions are located at least 100 kpc fro…

astro-ph2003

Gas outflows in radio galaxies

R. Morganti, T. Oosterloo, B. H. C. Emonts +2

We present a summary of our recent results on gas outflows in radio galaxies. Fast outflows (up to 2000 km/s) have been detected both in ionized and neutral gas. The latter is part…

astro-ph2003

HI on large and small scales in starburst radio galaxies

Raffaella Morganti, Tom Oosterloo, Clive Tadhunter +2

The study of the optical continuum of radio galaxies shows that about 30% have a young stellar population component. Among them are the most far-IR bright radio galaxies. A further…