R. Maiolino,1 S. Arribas,2 T. Boker,3 A. Bunker,4 S. Chariot,5 G. de Marchi,3 P. Ferruit,6 M. Franx,7 P. Jakobsen,3 H. Moseley,8 T. Nagao,9 L. Origlia,10 B. Rauscher,8 M. Regan,11 H. W. Rix12 &
1 INAF - Astronomical Observatory of Rome, Italy 2 CSIC - Departamento de Astrofísica Molecular e Infrarroja, Madrid, Spain 3 European Space Agency - ESTEC, Noordwijk, the Netherlands 4 School of Physics, University of Exeter, Exeter, UK 5 Institute d'Astrophysique de Paris, Paris, France 6 CRAL - Observatoire de Lyon, 9 Avenue Charles André, Saint-Genis Laval, France 7 Leiden Observatory, Leiden, the Netherlands 8 NASA - Goddard Space Flight Center, MD, USA 9 National Astronomical Observatory of Japan, Osawa, Japan 10 INAF - Astronomical Observatory of Bologna, Bologna, Italy 11 Space Telescope Science Institute, Baltimore, MD, USA 12 Max-Planck-Institut fur Astronomie, Heidelberg, Germany 13 Herzberg Institute of Astrophysics, Victoria, Canada
The James Webb Space Telescope is a 6.6-m-aperture, passively cooled space observatory optimized for near-IR observations. It will be one of the most important observing facilities in the next decade, and it is designed to address numerous outstanding issues in astronomy. In this article we focus specifically on its capabilities to investigate the chemical abundances of various classes of astronomical objects and their metallicity evolution through the cosmic epochs.
Was this article helpful?