Presentation + Paper
10 July 2018 Primary and secondary mirror manufacturing for COLIBRI ground follow-up telescope of the SVOM mission
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, F. Dolon
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); https://doi.org/10.1117/12.2311656
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Mirrors

Polishing

Wavefront sensors

Interferometry

RELATED CONTENT

INO340 active optics algorithm
Proceedings of SPIE (August 26 2022)
Overview and status of the Giant Magellan Telescope project
Proceedings of SPIE (December 13 2020)
The interferometric test bench for the ELT M2 polishing and...
Proceedings of SPIE (September 12 2021)
Visible MCAO channel for NIRVANA at the LBT
Proceedings of SPIE (February 07 2003)
LINC NIRVANA how to get a 23 m wavefront...
Proceedings of SPIE (October 25 2004)
Testing The Primary Mirror Of The W. M. Keck Observatory
Proceedings of SPIE (March 23 1987)
Submillimeter pupil-plane wavefront sensing
Proceedings of SPIE (July 15 2010)

Back to Top