91̽»¨

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding 91̽»¨
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
91̽»¨
Black Hole

Lensing of space time around a black hole. At 91̽»¨ 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

A Population of z>2 Far-Infrared Herschel-SPIRE selected Starbursts

(2012)

Authors:

CM Casey, S Berta, M Béthermin, J Bock, C Bridge, D Burgarella, E Chapin, SC Chapman, DL Clements, A Conley, CJ Conselice, A Cooray, D Farrah, E Hatziminaoglou, RJ Ivison, E Le Floc'h, D Lutz, G Magdis, B Magnelli, SJ Oliver, MJ Page, F Pozzi, D Rigopoulou, L Riguccini, IG Roseboom, DB Sanders, D Scott, N Seymour, I Valtchanov, JD Vieira, M Viero, J Wardlow

A Redshift Survey of Herschel Far-Infrared Selected Starbursts and Implications for Obscured Star Formation

(2012)

Authors:

CM Casey, S Berta, M Béthermin, J Bock, C Bridge, J Budynkiewicz, D Burgarella, E Chapin, SC Chapman, DL Clements, A Conley, CJ Conselice, A Cooray, D Farrah, E Hatziminaoglou, RJ Ivison, E Le Floc'h, D Lutz, G Magdis, B Magnelli, SJ Oliver, MJ Page, F Pozzi, D Rigopoulou, L Riguccini, IG Roseboom, DB Sanders, D Scott, N Seymour, I Valtchanov, JD Vieira, M Viero, J Wardlow

The molecular gas content of z = 3 lyman break galaxies: Evidence of a non-evolving gas fraction in main-sequence galaxies at z > 2

Astrophysical Journal Letters 758:1 (2012)

Authors:

GE Magdis, E Daddi, M Sargent, D Elbaz, R Gobat, H Dannerbauer, C Feruglio, Q Tan, D Rigopoulou, V Charmandaris, M Dickinson, N Reddy, H Aussel

Abstract:

We present observations of the CO[J = 3 → 2] emission toward two massive and infrared luminous Lyman break galaxies (LBGs) at z = 3.21 and z = 2.92, using the IRAM Plateau de Bure Interferometer, placing first constraints on the molecular gas masses (M gas) of non-lensed LBGs. Their overall properties are consistent with those of typical (main-sequence) galaxies at their redshifts, with specific star formation rates 1.6 and 2.2Gyr-1, despite their large infrared luminosities (L IR (2-3) × 1012L) derived from Herschel. With one plausible CO detection (spurious detection probability of 10-3) and one upper limit, we investigate the evolution of the molecular gas-to-stellar mass ratio (M gas/M *) with redshift. Our data suggest that the steep evolution of M gas/M * of normal galaxies up to z 2 is followed by a flattening at higher redshifts, providing 91̽»¨ing evidence for the existence of a plateau in the evolution of the specific star formation rate at z > 2.5. © 2012. The American Astronomical Society. All rights reserved.

The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy Distributions

(2012)

Authors:

Georgios E Magdis, E Daddi, M Bethermin, M Sargent, D Elbaz, M Pannella, M Dickinson, H Dannerbauer, E Da Cunha, F Walter, D Rigopoulou, V Charmandaris, H-S Hwang, J Kartaltepe

The Molecular Gas Content of z = 3 Lyman Break Galaxies; Evidence of a non Evolving Gas Fraction in Main Sequence Galaxies at z > 2

(2012)

Authors:

GE Magdis, E Daddi, M Sargent, D Elbaz, R Gobat, H Dannerbauer, Q Tan, C Feruglio, D Rigopoulou, V Charmandaris, M Dickinson, N Reddy, H Aussel

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 52
  • Page 53
  • Page 54
  • Page 55
  • Current page 56
  • Page 57
  • Page 58
  • Page 59
  • Page 60
  • …
  • Next page Next
  • Last page Last

Footer 91̽»¨

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

91̽»¨,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

© 91̽»¨ - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics