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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
  • Research
  • Publications

ISOCAM-CVF 5-12 micron spectroscopy of ultraluminous infrared galaxies

ASTROPHYSICAL JOURNAL 552:2 (2001) 527-543

Authors:

QD Tran, D Lutz, R Genzel, D Rigopoulou, HWW Spoon, E Sturm, M Gerin, DC Hines, AFM Moorwood, DB Sanders, N Scoville, Y Taniguchi, M Ward
More details from the publisher

The European Large Area ISO Survey -: IV.: The preliminary 90-μm luminosity function

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 322:2 (2001) 262-268

Authors:

S Serjeant, A Efstathiou, S Oliver, C Surace, P Héraudeau, MJD Linden-Vornle, C Gruppioni, F La Franca, D Rigopoulou, T Morel, H Crockett, T Sumner, M Rowan-Robinson, M Graham
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The European Large-Area Infrared Space Observatory Survey V:: a BeppoSax hard X-ray survey of the S1 region

ASTROPHYSICAL JOURNAL 554:1 (2001) 18-26

Authors:

DM Alexander, F La Franca, F Fiore, X Barcons, P Ciliegi, L Danese, R Della Ceca, A Franceschini, C Gruppioni, G Matt, I Matute, S Oliver, F Pompilio, A Wolter, A Efstathiou, P Héraudeau, GC Perola, M Perri, D Rigopoulou, M Rowan-Robinson, S Serjeant
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The extended counterpart of submm source Lockman 850.1

ASTRONOMY & ASTROPHYSICS 378:1 (2001) 70-75

Authors:

D Lutz, JS Dunlop, O Almaini, P Andreani, A Blain, A Efstathiou, M Fox, R Genzel, G Hasinger, D Hughes, RJ Ivison, A Lawrence, RG Mann, S Oliver, JA Peacock, D Rigopoulou, M Rowan-Robinson, S Scott, S Serjeant, L Tacconi
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The nature of ISOCAM galaxies in the Hubble Deep Field South

SPRINGER PROC PHYS 88 (2001) 255-260

Authors:

D Rigopoulou, A Franceschini, R Genzel

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. Here we report results of our near-infrared VLT-ISAAC spectroscopic survey aimed at characterising the nature of these sources. We find that the rest-frame R-band spectra resemble those of powerful dust enshrouded starbursts. More recent detailed studies revealed that some of these systems are in fact extremely massive galaxies.
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