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20072026
most citedThe James Webb Space Telescope Mission

490 citations · 3.5k across the 72 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 60 cited

The origin of the infrared emission in radio galaxies II: analysis of mid- to far-infrared Spitzer observations of the 2Jy sample

D. Dicken, C. Tadhunter, D. Axon +5

We present an analysis of deep mid- to far-infrared (MFIR) Spitzer photometric observations of the southern 2Jy sample of powerful radio sources (0.05 < z < 0.7), conducting a stat…

astro-ph2008★ 45 cited

The origin of the infrared emission in radio galaxies I: new mid- to far-infrared and radio observations of the 2Jy sample

D. Dicken, C. Tadhunter, R. Morganti +3

As part of a large study to investigate the nature of the longer wavelength continuum emission of radio-loud AGN, we present new mid to far-infrared (MFIR) and high frequency radio…

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

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-ph2007★ 39 cited

The heating mechanism for the warm/cool dust in powerful, radio-loud AGN

C. Tadhunter, D. Dicken, J. Holt +7

The uncertainty surrounding the nature of the heating mechanism for the dust that emits at mid- to far-IR (MFIR) wavelengths in active galaxies limits our understanding of the link…