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Brigitte Rocca-Volmerange
Researcher at Institut d'Astrophysique de Paris
Publications - 75
Citations - 9662
Brigitte Rocca-Volmerange is an academic researcher from Institut d'Astrophysique de Paris. The author has contributed to research in topics: Galaxy & Radio galaxy. The author has an hindex of 29, co-authored 75 publications receiving 8327 citations. Previous affiliations of Brigitte Rocca-Volmerange include Goddard Space Flight Center & University of Paris-Sud.
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Journal ArticleDOI
Merging history trees of dark matter haloes: a tool for exploring galaxy formation models
TL;DR: In this paper, a method of deriving and using merging history trees of dark matter galaxy haloes directly from pure gravity N-body simulations is presented, which combines the full nonlinearity of Nbody simulations with the flexibility of the semi-analytical approach.
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Rapid coeval black hole and host galaxy growth in MRC 1138-262: the hungry spider
Nick Seymour,Nick Seymour,Bruno Altieri,C. De Breuck,Pieter Barthel,D. Coia,L. Conversi,Helmut Dannerbauer,Arjun Dey,Mark Dickinson,Guillaume Drouart,Guillaume Drouart,Audrey Galametz,Thomas R. Greve,Martin Haas,Nina A. Hatch,Edo Ibar,Rob Ivison,Rob Ivison,Matt J. Jarvis,Matt J. Jarvis,Attila Kovács,Jaron Kurk,Matt Lehnert,George K. Miley,Nicole P. H. Nesvadba,J. I. Rawlings,Alessandro Rettura,H. J. A. Röttgering,Brigitte Rocca-Volmerange,Miguel Sánchez-Portal,J. S. Santos,Daniel Stern,Jason R. Stevens,I. Valtchanov,Joel Vernet,Dominika Wylezalek +36 more
TL;DR: In this article, a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC1138-26 at z = 2.156, also known as the Spiderweb Galaxy, was presented.
Journal Article
Pegase: A UV to NIR spectral evolution model of galaxies. Application to the calibration of bright galaxy counts
TL;DR: PEGASE as discussed by the authors is a new spectrophotometric evolution model for starbursts and evolved galaxies of the Hubble sequence, which is coherently linked to the visible and the ultraviolet (UV) so that the model is continuous on an exceptionally large wavelength range from 220 A up to 5 μm.
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The European Large Area ISO Survey III: 90micron extragalactic source counts
Andreas Efstathiou,S. J. Oliver,Michael Rowan-Robinson,Christian Surace,T. J. Sumner,P. Heraudeau,M. Linden-Vørnle,D. Rigopoulou,Steve Serjeant,Robert G. Mann,C. J. Cesarsky,L. Danese,Alberto Franceschini,R. Genzel,Andy Lawrence,Dietrich Lemke,R. G. McMahon,G. K. Miley,Brigitte Rocca-Volmerange +18 more
TL;DR: In this paper, the authors presented results and source counts at 90micron extracted from the Preliminary Analysis of the European Large Area ISO Survey (ELAIS) and showed that the majority of the detected sources are associated with galaxies on optical images.
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Jet and torus orientations in high redshift radio galaxies
Guillaume Drouart,Guillaume Drouart,Guillaume Drouart,C. De Breuck,Joel Vernet,Robert Laing,Nick Seymour,Daniel Stern,Martin Haas,E. A. Pier,Brigitte Rocca-Volmerange +10 more
TL;DR: In this article, the relative orientation of radio jets and dusty tori surrounding the active galactic nucleus (AGN) in powerful radio galaxies at z ǫ > 1.3 was examined.