Project Details
The role of galaxy environment on the star forming intensity of high-redshift radio sources
Applicant
Professor Dr. Rolf Chini, since 8/2019
Subject Area
Astrophysics and Astronomy
Term
from 2015 to 2023
Project identifier
Deutsche Forschungsgemeinschaft (DFG) - Project number 289328479
During the cosmic era of maximum star formation, radio sources show a broad range of star formation activity in their host galaxies. We aim to check the hypothesis that the star forming intensity is controlled by the environment of the radio sources. This is important for understanding the physical processes that turn star formation on (mergers) and off (AGN-driven quenching).Using the Herschel and Spitzer Space Telescopes, we have mapped the complete 3CR sample of 64 radio galaxies and quasars at high redshift (1
DFG Programme
Research Grants
International Connection
Netherlands, United Kingdom, USA
Cooperation Partners
Professor Dr. Peter Barthel; Dr. Carlos De Breuck; Dr. Marco Chiaberge; Dr. Dave Clements; Professor Dr. Klaus Winfried Meisenheimer (†); Professor Dr. George K. Miley; Dr. Pece Podigachoski; Dr. Daniel Stern; Dr. Belinda Wilkes; Dr. Steve Willner
Ehemaliger Antragsteller
Privatdozent Dr. Martin Haas, until 8/2019