Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
Test image

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
  • About
  • Research
  • Gresham Professorship
  • Books
  • Teaching
  • Prizes
  • Publications

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

(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

ArXiv astro-ph/9704163 (1997)

Authors:

Chris J Willott, Steve Rawlings, Katherine M Blundell, Mark Lacy

Abstract:

We present details of a new sample of radio-loud quasars drawn from 0.013 sr of the 7C Redshift Survey. This sample is small (21 quasars) but complete in that every object with an unresolved nucleus and/or broad emission lines with S(151MHz) > 0.5 Jy has been discovered. The dependence of the quasar fraction with redshift and radio luminosity is investigated, providing new evidence supporting the unification of radio-loud quasars and powerful radio galaxies. This 7C sample is compared with optically-selected quasars, in order to determine whether there are systematic biases in the different selection techniques. There are no lightly reddened (Av approx. 1) quasars in our sample amongst the 14 with z < 2. The discovery of a reddened quasar at z = 2.034 and its implications are discussed. A tight correlation between radio luminosity and optical/near infrared continuum luminosity for a subset of the sample is also found.
Details from ArXiV
More details from the publisher
Details from ORA
More details

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
More details from the publisher

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.
Details from ArXiV
More details from the publisher

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 79
  • Page 80
  • Page 81
  • Page 82
  • Current page 83
  • Page 84
  • Page 85
  • Page 86
  • Page 87
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet