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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Prof Chris Lintott

Professor of Astrophysics and Citizen Science Lead

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Zooniverse
  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Rubin-LSST
chris.lintott@physics.ox.ac.uk
Telephone: 01865 (2)73638
Denys Wilkinson Building, room 532C
www.zooniverse.org
orcid.org/0000-0001-5578-359X
  • About
  • Citizen science
  • Group alumni
  • Publications

Zooniverse labs

Zooniverse lab
Build your own Zooniverse project

The Zooniverse lab lets anyone build their own citizen science project

Zooniverse Lab

Moon Zoo: Citizen science in lunar exploration

Astronomy and Geophysics 52:2 (2011) 2.10-2.12

Authors:

K Joy, I Crawford, P Grindrod, C Lintott, S Bamford, A Smith, A Cook, M Zoo

Abstract:

The Moon Zoo Team describe how citizen scientists can get involved and explore the Moon online. © 2011 Royal Astronomical Society.
More details from the publisher

Galaxy Zoo: Bar lengths in local disc galaxies

Monthly Notices of the Royal Astronomical Society (2011)

Authors:

B Hoyle, KL Masters, RC Nichol, EM Edmondson, AM Smith, C Lintott, R Scranton, S Bamford, K Schawinski, D Thomas
Details from ArXiV

Moon Zoo: citizen science in lunar exploration

ASTRONOMY & GEOPHYSICS 52:2 (2011) 10-12

Authors:

Katherine H Joy, Ian A Crawford, Peter M Grindrod, Chris Lintott, Steven Bamford, Arfon Smith, Anthony Cook
More details from the publisher

Reinventing Discovery: The New Era of Networked Science

NATURE 478:7369 (2011) 320-321
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The sudden death of the nearest quasar

Astrophysical Journal Letters 724:1 PART 2 (2010)

Authors:

K Schawinski, DA Evans, S Virani, CM Urry, WC Keel, P Natarajan, CJ Lintott, A Manning, P Coppi, S Kaviraj, SP Bamford, GIG Józsa, M Garrett, H Van Arkel, P Gay, L Fortson

Abstract:

Galaxy formation is significantly modulated by energy output from supermassive black holes at the centers of galaxies which grow in highly efficient luminous quasar phases. The timescale on which black holes transition into and out of such phases is, however, unknown. We present the first measurement of the shutdown timescale for an individual quasar using X-ray observations of the nearby galaxy IC 2497, which hosted a luminous quasar no more than 70,000 years ago that is still seen as a light echo in "Hanny's Voorwerp," but whose present-day radiative output is lower by at least two, and more likely by over four, orders of magnitude. This extremely rapid shutdown provides new insight into the physics of accretion in supermassive black holes and may signal a transition of the accretion disk to a radiatively inefficient state. © 2010. The American Astronomical Society. All rights reserved.
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