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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.

Michele Cappellari

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • Extremely Large Telescope
michele.cappellari@physics.ox.ac.uk
Telephone: 01865 (2)73647
Denys Wilkinson Building, room 755
  • About
  • Publications

The counterrotating core and the black hole mass of IC1459

(2002)

Authors:

M Cappellari, EK Verolme, RP van der Marel, GA Verdoes Kleijn, GD Illingworth, M Franx, CM Carollo, PT de Zeeuw
More details from the publisher

Efficient Multi-Gaussian Expansion of galaxies

(2002)
More details from the publisher

A SAURON study of M32: measuring the intrinsic flattening and the central black hole mass

(2002)

Authors:

EK Verolme, M Cappellari, Y Copin, RP van der Marel, R Bacon, M Bureau, RL Davies, BM Miller, PT de Zeeuw
More details from the publisher

A SAURON study of M32: measuring the intrinsic flattening and the central black hole mass

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 335:3 (2002) 517-525

Authors:

EK Verolme, M Cappellari, Y Copin, RP van der Marel, R Bacon, M Bureau, RL Davies, BM Miller, PT de Zeeuw
More details from the publisher

Adaptive spatial binning of 2D spectra and images using Voronoi Tessellations

ASTR SOC P 282 (2002) 515-522

Authors:

M Cappellari, Y Copin

Abstract:

We present new techniques to perform adaptive spatial binning of two-dimensional (2D) data to reach a chosen constant signal-to-noise ratio per bin. These methods are required particularly for the proper analysis of Integral Field Spectrograph (IFS) observations, but can also be used for standard photometric imagery. Various schemes axe tested and compared using data obtained with the panoramic IFS SAURON.
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