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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. Dimitra Rigopoulou

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
Dimitra.Rigopoulou@physics.ox.ac.uk
Telephone: 01865 (2)73296
Denys Wilkinson Building, room 75419514947
  • About
  • Publications

Infrared spectroscopy of faint 15 micron sources in the Hubble Deep Field South: first hints at the properties of the sources of the IR background

(2003)

Authors:

A Franceschini, S Berta, D Rigopoulou, H Aussel, CJ Cesarsky, D Elbaz, R Genzel, E Moy, S Oliver, M Rowan-Robinson, PP Van der Werf
More details from the publisher

H-band observations of the Chandra Deep Field South

ASTRONOMY & ASTROPHYSICS 403:2 (2003) 493-499

Authors:

E Moy, P Barmby, D Rigopoulou, JS Huang, SP Willner, GG Fazio
More details from the publisher

ISO observations of four active galaxies

ASTRONOMY & ASTROPHYSICS 406:2 (2003) 527-534

Authors:

M Dennefeld, T Boller, D Rigopoulou, HWW Spoon
More details from the publisher

Infrared spectroscopy of faint 15 μm sources in the Hubble Deep Field South:: First hints at the properties of the sources of the IR background

ASTRONOMY & ASTROPHYSICS 403:2 (2003) 501-522

Authors:

A Franceschini, S Berta, D Rigopoulou, H Aussel, CJ Cesarsky, D Elbaz, R Genzel, E Moy, S Oliver, M Rowan-Robinson, PP Van der Werf
More details from the publisher

Kinematics of ISOCAM selected star-forming galaxies at z similar to 1 in the Hubble Deep Field

ESO ASTROPHY SYMP (2003) 232-237

Authors:

D Rigopoulou, A Franceschini, R Genzel, N Thatte

Abstract:

The various deep ISOCAM surveys revealed a new class of infrared luminous galaxies which are characterized by a high rate of evolution and are found at redshifts of zsimilar to1. Based on our near-infrared low-resolution spectroscopy we find that these ISOCAM galaxies are dust-enshrouded star-forming galaxies. Here we report on the first spatially resolved H. velocity profiles of ISOCAM galaxies in the Hubble Deep Field South. We find that some of these systems are in fact extremely massive galaxies. The galaxies show an offset of 1.6+/-0.3 magnitude in the rest frame B-band when compared to the local Tully-Fisher relation.
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