10 July 2018 Primary and secondary mirror manufacturing for COLIBRI ground follow-up telescope of the SVOM mission
Author Affiliations +
Abstract
COLIBRI is one of the two robotic ground follow-up telescopes for the SVOM (Space Variable Object Monitor) mission dedicated to the study of gamma-ray bursts, allowing determination of precise celestial coordinates of the detected bursts. COLIBRI telescope is a two-mirror Ritchey-Chrétien telescope whose concave primary and convex secondary mirrors have diameters of 1325mm and 485mm respectively. The mirrors are currently manufactured at LAM (Laboratoire d’Astrophysique de Marseille). In this article, the advancement of the work is presented. We also give a global overview and status of the COLIBRI project.
Conference Presentation
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. Floriot, M. Marcos, J. Fuentes-Fernandez, A. M. Watson, S. Cuevas Cardona, W. H. Lee, S. Basa, D. Corre, M. Ferrari, E. Hugot, K. Dohlen, F. A. Uribe, A. F. Simon, R. L. Lebre, E. Jimenez-Bailon, J. L. Ochoa, F. Quiros, E. Cadena, L. Figueroa, E. Pallier, J. Platzer, A. Klotz, J. L. !!!!!!!!Attéia, H. Valentin, R. Mathon, J. Boy, P. Ambert, J. F. Le Borgne, D. Dornic, C. Meessen, M. Ageron, O. Boulade, B. Cordier, D. Dubreuil, S. Ronayette, P. Gallais, A. Le Van Suu, P. E. Blanc, and F. Dolon "Primary and secondary mirror manufacturing for COLIBRI ground follow-up telescope of the SVOM mission", Proc. SPIE 10706, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III, 107060M (10 July 2018); doi: 10.1117/12.2311656; https://doi.org/10.1117/12.2311656
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