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Katherine Blundell OBE

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Plasma physics

Sub department

  • Astrophysics

Research groups

  • Global Jet Watch
  • Pulsars, transients and relativistic astrophysics
Katherine.Blundell@physics.ox.ac.uk
Telephone: 01865 (2)73308
Denys Wilkinson Building, room 707
www.GlobalJetWatch.net
orcid.org/0000-0001-8509-4939
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The Global Jet Watch

Radio image of the microquasar SS433
The micro quasar SS433
Link to the site

A sample of 6C radio sources designed to find objects at redshift > 4: the radio data

ArXiv astro-ph/9707336 (1997)

Authors:

Katherine M Blundell, Steve Rawlings, Stephen A Eales, Gregory B Taylor, Alistair D Bradley

Abstract:

We describe the selection of a sample of 34 radio sources from the 6C survey (Hales, Baldwin & Warner 1993) from a region of sky covering 0.133 sr. The selection criteria for this sample, hereafter called 6C*, were chosen to optimise the chances of finding radio galaxies at redshift z > 4. Optical follow-up observations have already led to the discovery of the most distant known radio galaxy at z = 4.41 (Rawlings et al. 1996). We present VLA radio maps and derive radio spectra for all the 6C* objects.
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A sample of 6C radio sources designed to find objects at redshift > 4: the radio data

(1997)

Authors:

Katherine M Blundell, Steve Rawlings, Stephen A Eales, Gregory B Taylor, Alistair D Bradley
More details from the publisher

A complete sample of quasars from the 7C redshift survey

(1997)

Authors:

Chris J Willott, Steve Rawlings, Katherine M Blundell, Mark Lacy
More details from the publisher

Cosmology with redshift surveys of radio sources

(1997)

Authors:

Steve Rawlings, Katherine M Blundell, Mark Lacy, Chris J Willott, Stephen A Eales
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Evidence for a black hole in a radio-quiet quasar nucleus

ArXiv astro-ph/9606102 (1996)

Authors:

Katherine M Blundell, Anthony J Beasley, Mark Lacy, Simon Garrington

Abstract:

We present the first milli-arcsecond resolution radio images of a radio-quiet quasar, detecting a high brightness temperature core with data from the VLBA. On maps made with lower-frequency data from MERLIN and the VLA jets appear to emanate from the core in opposite directions, which correspond to radio-emission on arcsecond scales seen with the VLA at higher frequencies. These provide strong evidence for a black-hole--based jet-producing central engine, rather than a starburst, being responsible for the compact radio emission in this radio-quiet quasar.
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