Year: 2016
Type: article
Abstract: Context. The star formation rate is a crucial parameter for the investigation galaxy evolution. At low redshift the cosmic star formation rate density declines smoothly, and massive active galaxies become passive, reducing their star formation activity. This implies that the bulk of the star formation rate density at low redshift is mainly driven by low mass objects.
Source: Astronomy and Astrophysics
Institutions: University of Lisbon, Institute of Astrophysics and Space Sciences, Max Planck Institute for Extraterrestrial Physics, Universidad Nacional Autónoma de México, Centre National de la Recherche Scientifique, Aix-Marseille Université, Laboratoire d’Astrophysique de Marseille, Universidad de Antofagasta, University of Cambridge, Ghent University, University of Crete, Arcetri Astrophysical Observatory, Osservatorio Astronomico di Padova, University of Manchester, University College London, Cardiff University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Funders: National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Alfred P. Sloan Foundation, Yale University, Vanderbilt University, Princeton University, Ohio State University, California Institute of Technology, Harvard University, University of Washington, Johns Hopkins University, University of Arizona, Carnegie Mellon University, University of Portsmouth, New Mexico State University, UK Space Agency, York University, Imperial College London, Cardiff University, Centre National d’Etudes Spatiales, Centre National de la Recherche Scientifique, Office of Science, College of Engineering, Michigan State University, Science and Technology Facilities Council, Fundação para a Ciência e a Tecnologia, National Astronomical Observatories, Chinese Academy of Sciences, Brookhaven National Laboratory, Lawrence Berkeley National Laboratory
Awards: Em busca de galáxias longínquas na época da reionização com o ALMA, UK ALMA Regional Centre Node Support: 2016 - 2020, Support for the UK ALMA Regional Centre Node, Projecto Estratégico - UI 2751 - 2014, DUST AS A PROBE OF GALACTIC ENVIRONMENT, Instituto de Astrofísica e Ciências do Espaço, UCL Astrophysics Consolidated Grant 2015-2018
OpenAlex ID: W4297943536