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20012012
most citedThe bulk of the black hole growth since z~1 occurs in a secular universe: No major merger-AGN connection

404 citations · 1.3k across the 22 of their papers we have counts for

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11 papers · 1 filter

astro-ph2008★ 27 cited

PKS2250-41: a case study for triggering

K. J. Inskip, M. Villar-Martin, C. N. Tadhunter +3

We present the results of a multiwavelength study of the z = 0.31 radio source PKS2250-41. Integral field unit and long-slit spectroscopy obtained using VIMOS and FORS1 on the VLT,…

astro-ph2007★ 15 cited

PKS1932-46: a radio source in an interacting group?

K. J. Inskip, C. N. Tadhunter, D. Dicken +3

We present the results of a multiwavelength study of the z=0.23 radio source PKS1932-46. VIMOS IFU spectroscopy is used to study the morphology, kinematics and ionisation state of…

astro-ph2007★ 69 cited

The properties of the young stellar populations in powerful radio galaxies at low and intermediate redshifts

J. Holt, C. N. Tadhunter, R. M. Gonzalez Delgado +5

Abridged. We present high-quality optical spectra for 12 powerful radio sources at low and intermediate redshifts (z < 0.7) that show evidence for a substantial UV excess. These da…

astro-ph2007

VIMOS spectroscopy of extended emission line regions

K. J. Inskip, M. Villar-Martin, C. Tadhunter +3

We present the results of spectroscopic and imaging observations of the FRII radio galaxies PKS2250-41 and PKS1932-46. Both sources display very extensive emission line regions, an…

astro-ph2006★ 6 cited

Deep spectroscopy of 9C J1503+4528: a very young CSS radio source at z=0.521

K. J. Inskip, D. Lee, Garret Cotter +7

9C J1503+4528 is a very young CSS radio galaxy, with an age of order 10^4 years. This source is therefore an ideal laboratory for the study ofthe intrinsic host galaxy/IGM properti…

astro-ph2005★ 10 cited

Deviations from passive evolution - star formation and the UV excess in z~1 radio galaxies

K. J. Inskip, P. N. Best, M. S. Longair

Galaxy colours are determined for two samples of 6C and 3CR radio sources at z~1, differing by a factor of ~6 in radio power. Corrections are made for emission line contamination a…