The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope - IV. Capabilities and predicted performance for exoplanet characterization

Summary

This is a publication. If there is no link to the publication on this page, you can try the pre-formated search via the search engines listed on this page.

Authors: S. M. Birkmann, P. Ferruit, G. Giardino, L. D. Nielsen, A. García Muñoz, S. Kendrew, B. J. Rauscher, T. L. Beck, C. Keyes, J. A. Valenti, P. Jakobsen, B. Dorner, C. Alves de Oliveira, S. Arribas, T. Böker, A. J. Bunker, S. Charlot, G. de Marchi, N. Kumari, M. López-Caniego, N. Lützgendorf, R. Maiolino, E. Manjavacas, A. Marston, S. H. Moseley, N. Prizkal, C. Proffitt, T. Rawle, H.-W. Rix, M.

Journal title: Astronomy & Astrophysics

Journal number: 661

Journal publisher: Springer Verlag

Published year: 2022

Published pages: A83

DOI identifier: 10.1051/0004-6361/202142592

ISSN: 0004-6361