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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

A 15 mu m selected sample of high-z starbursts and AGNs

ASTR SOC P 381 (2008) 367-371

Authors:

A Hernan-Caballero, I Perez-Fournon, M Rowan-Robinson, D Rigopoulou, A Afonso-Luis, E Hatziminaoglou, E Gonzalez-Solares, FM Montenegro-Montes, B Vila-Vilaro, D Farrah, C Lari, M Vaccari, T Babbedge, S Oliver, D ClementS, S Serjeant, F Pozzi, F La Franca, C Gruppioni, I Valtchanov, C Lonsdale, SWIRE Team

Abstract:

We report results from our Spitzer GO-1 program on IRS spectroscopy of a large sample of Luminous Infrared Galaxies and quasars selected from the European Large Area ISO Survey (ELAIS). The selected ELAIS sources have a wide multi-wavelength coverage, including ISOCAM, ISOPHOT, IRAC and MIPS (from SWIRE), and optical photometry. Here we present the sample selection and results from the IRS spectroscopy.
More details

Follow-up NIR spectroscopy of ULIRGs observed by ISO

ASTR SOC P 381 (2008) 275-278

Authors:

H Dannerbauer, D Rigopoulou, D Lutz, R Genzel, E Sturm, AFM Moorwood

Abstract:

We discuss low resolution near-infrared spectroscopy of an unbiased sample of 24 ultraluminous infrared galaxies (ULIRGs), selected from samples previously observed in the mid-infrared with ISO. Qualitatively, the NIR spectra of our 24 ULIRGs resemble those of starbursts. The spectroscopic classification in the NIR is in very good agreement with the MIR. For a subset of our sample for which extinction corrections can be derived from Pace and Br gamma, we find rather high Pa alpha luminosities, in accordance with the powering source of these galaxies being star formation. Furthermore, we identified two unusual objects, the first exhibiting extreme [FeII] emission and the second strong emission in H-2 rotation-vibration emission.
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IRAC photometric analysis and the mid-IR photometric properties of Lyman-break galaxies

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 386:1 (2008) 11-21

Authors:

GE Magdis, D Rigopoulou, J-S Huang, GG Fazio, SP Willner, MLN Ashby
More details from the publisher

The host galaxies and black holes of typical z ∼ 0.5-1.4 AGNs

ASTROPHYSICAL JOURNAL 677:1 (2008) 127-136

Authors:

Almudena Alonso-Herrero, Pablo G Perez-Gonzalez, George H Rieke, David M Alexander, Jane R Rigby, Casey Papovich, Jennifer L Donley, Dimitra Rigopoulou
More details from the publisher
Details from ArXiV

The Host Galaxies and Black Holes of Typical z~0.5-1.4 AGN

(2007)

Authors:

A Alonso-Herrero, PG Perez-Gonzalez, GH Rieke, DM Alexander, JR Rigby, C Papovich, JL Donley, D Rigopoulou
More details from the publisher

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