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papers

Publications (29)

astro-ph2005

Nuclear Properties of Nearby Spiral Galaxies from Hubble Space Telescope NICMOS imaging and STIS Spectroscopy

M. A. Hughes, D. Axon, J. Atkinson +16

astro-ph.HE2009

Polarimetry and the High-Energy Emission Mechanisms in Quasar Jets

M. Cara, E. S. Perlman, Y. Uchiyama +15

astro-ph2003

Spectroscopy of the near-nuclear regions of Cygnus A: estimating the mass of the supermassive black hole

C. Tadhunter, A. Marconi, D. Axon +3

astro-ph.GA2014

Spitzer Mid-IR Spectroscopy of Powerful 2Jy and 3CRR Radio Galaxies. II. AGN Power Indicators and Unification

D. Dicken, C. Tadhunter, R. Morganti +14

astro-ph1999

PKS2250-41 and the role of jet-cloud interactions in powerful radio galaxies

M. Villar-Martin, C. Tadhunter, R. Morganti +2

astro-ph.CO2009

The Nature of the Near-IR Core Source in 3C 433

Edgar A. Ramirez, C. N. Tadhunter, D. Axon +4

astro-ph2008

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

astro-ph2000

Sub-mm and X-ray background: two unrelated phenomena?

P. Severgnini, R. Maiolino, M. Salvati +9

astro-ph1999

PKS2250-41 and the role of jet-cloud interactions in powerful radio galaxies (full paper)

M. Villar-Martin, C. Tadhunter, R. Morganti +2

astro-ph1994

Nuclear bars and blue nuclei within barred spiral galaxies

M. Shaw, D. Axon, R. Probst +1

astro-ph2000

The large scale distribution of warm ionized gas around nearby radio galaxies with jet-cloud interactions

C. N. Tadhunter, M. Villar-Martin, R. Morganti +2

astro-ph2006

Resolving the BLR in NGC 3783

P. Lira, M. Kishimoto, A. Robinson +5

astro-ph1998

PKS 1932-464: a jet-cloud interaction in a radio galaxy?

M. Villar-Martin, C. N. Tadhunter, R. Morganti +3

astro-ph.GA2014

Near-infrared Hubble Space Telescope polarimetry of a complete sample of narrow-line radio galaxies

E. A. Ramírez, C. N. Tadhunter, D. Axon +5

astro-ph2008

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

astro-ph.HE2010

Chandra Observations of 3C Radio Sources with z<0.3: Nuclei, Diffuse Emission, Jets and Hotspots

F. Massaro, D. E. Harris, G. Tremblay +11

astro-ph.GA2014

HST and Spitzer point source detection and optical extinction in powerful narrow-line radio galaxies

E. A. Ramírez, C. N. Tadhunter, D. Dicken +4

astro-ph2007

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

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

astro-ph.CO2009

On the observed distributions of black hole masses and Eddington ratios from radiation pressure corrected virial indicators

A. Marconi, D. Axon, R. Maiolino +5

astro-ph.CO2010

The origin of the infrared emission in radio galaxies. III. Analysis of 3CRR objects

D. Dicken, C. Tadhunter, D. Axon +3

astro-ph2004

Nuclear properties of a sample of nearby spirals from STIS imaging

C. Scarlata, M. Stiavelli, M. Hughes +17

astro-ph.HE2012

Chandra Observations of 3C Radio Sources with z<0.3 II: completing the snapshot survey

F. Massaro, G. R. Tremblay, D. E. Harris +14

astro-ph2000

The black hole mass vs bulge mass relationship in spiral galaxies

A. Marconi, D. Axon, J. Atkinson +15

astro-ph2005

Integral Field Spectroscopy of 23 Spiral Bulges

D. Batcheldor, D. Axon, D. Merritt +7

astro-ph.CO2011

Spitzer mid-IR spectroscopy of powerful 2Jy and 3CRR radio galaxies. I. Evidence against a strong starburst-AGN connection in radio-loud AGN

D. Dicken, C. Tadhunter, D. Axon +9

astro-ph.CO2010

Spectroastrometry of rotating gas disks for the detection of supermassive black holes in galactic nuclei. I. Method and simulations

A. Gnerucci, A. Marconi, A. Capetti +2

astro-ph2006

The NICMOS Polarimetric Calibration

D. Batcheldor, A. Robinson, D. Axon +3

astro-ph2001

HST observations of NGC 6240

J. Gerssen, R. P. van der Marel, D. Axon +3

astro-ph2008

Weighing black holes from zero to high redshift

A. Marconi, D. Axon, R. Maiolino +4