475 citations · 1.5k across the 27 of their papers we have counts for
25 papers
Lyman and Balmer breaks reveal mature z=8 galaxies with the code Pegase.3
Brigitte Rocca-Volmerange, A. Hilberer, M. Fioc
The z=8 galaxy sample (EGSY-2008532660, EGS-zs8-1, EGS-zs8-2), observed with HST and Spitzer/IRAC, was selected for its atypical [3.6]-[4.5]mum IR excess. The best-fitting of obser…
Disentangling star formation and AGN activity in powerful infrared luminous radio galaxies at 1<z<4
Guillaume Drouart, Brigitte Rocca-Volmerange, Carlos De Breuck +5
High-redshift radio galaxies present signs of both star formation and AGN activity, making them ideal candidates to investigate the connection and coevolution of AGN and star forma…
Supernova remnant mass cumulated along the star formation history of the z=3.8 radiogalaxies 4C41.17 and TN J2007-1316
Brigitte Rocca-Volmerange, Guillaume Drouart, Carlos De Breuck
In this paper, we show that the supernova remnant (SNR) masses cumulated from core-collapse supernovae along the star formation history of two powerful z=3.8 radio galaxies 4C41.17…
Rapidly growing black holes and host galaxies in the distant Universe from the Herschel Radio Galaxy Evolution Project
G. Drouart, C. De Breuck, J. Vernet +14
We present results from a survey of 70 radio galaxies (RGs) at redshifts 1<z<5.2 using the PACS and SPIRE on-board Herschel. Combined with existing mid-IR photometry from Spitzer a…
Starburst and old stellar populations in two z=3.8 radio galaxies 4C 41.17 and TN J2007-1316
Brigitte Rocca-Volmerange, Guillaume Drouart, Carlos De Breuck +6
The new evolutionary code Pegase.3 is used for the spectral synthesis of continuous optical-Spitzer-Herschel-submm spectral energy distributions (SEDs) of two z=3.8 radio galaxies…
Rapid Coeval Black Hole and Host Galaxy Growth in MRC 1138-262: The Hungry Spider
N. Seymour, B. Altieri, C. De Breuck +30
We present a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC 1138-26 at z = 2.156, also known as the Spiderweb Galaxy. By combinin…