activity
19982017
most citedObservations of HI Absorbing Gas in Compact Radio Sources at Cosmological Redshifts

137 citations · 722 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2017★ 17 cited

Investigating the Unification of LOFAR-detected powerful AGN in the Boötes Field

Leah K. Morabito, W. L. Williams, Kenneth J. Duncan +17

Low radio frequency surveys are important for testing unified models of radio-loud quasars and radio galaxies. Intrinsically similar sources that are randomly oriented on the sky w…

astro-ph.GA2017★ 48 cited

Radiative age mapping of the remnant radio galaxy B2 0924+30: the LOFAR perspective

A. Shulevski, R. Morganti, J. J. Harwood +9

We have observed the steep spectrum radio source B2 0924+30 using the LOw Frequency ARray (LOFAR) telescope. Hosted by a z=0.026 elliptical galaxy, it has a relatively large angula…

astro-ph.GA2015★ 3 cited

The far-infrared emission of the radio-loud quasar 3C318

P. Podigachoski, P. D. Barthel, R. F. Peletier +1

3C318, a radio-loud quasar at z=1.574, is a subgalactic-sized radio source, and a good test-bed for the interplay between black hole and galaxy growth in the high-z Universe. Based…

astro-ph.GA2015★ 9 cited

ALMA unveils a triple merger and gas exchange in a hyper-luminous radio galaxy at z=2: the Dragonfly Galaxy (II)

B. H. C. Emonts, C. De Breuck, M. D. Lehnert +9

The Dragonfly Galaxy (MRC0152-209), at redshift z~2, is one of the most vigorously star-forming radio galaxies in the Universe. What triggered its activity? We present ALMA Cycle 2…

astro-ph.GA2015★ 66 cited

Star formation in z>1 3CR host galaxies as seen by Herschel

P. Podigachoski, P. D. Barthel, M. Haas +15

We present Herschel (PACS and SPIRE) far-infrared (FIR) photometry of a complete sample of z>1 3CR sources, from the Herschel GT project The Herschel Legacy of distant radio-loud A…

astro-ph.CO2013★ 40 cited

Deep, wide-field, global VLBI observations of the Hubble Deep Field North and Flanking Fields

S. Chi, P. D. Barthel, M. A. Garrett

Dust is commonly present in weakly radio emitting star-forming galaxies and this dust may obscure the signatures of accreting black holes in these objects. We aim to uncover weak a…