COLIBRI, a wide-field 1.3 m robotic telescope dedicated to the transient sky


Por: Basa S., Lee W.H., Dolon F., Watson A.M., Floriot J., Atteia J.-L., Butler N.R., Dornic D., Lombardo S., Ronayette S., Ageron M., Agneray F., Ángeles F., Bautista L., Benamar-Aissa H., Blanpain C., Boulade O., Boy J., Buat V., Cadena E., Cuevas S., Farah A., Figueroa L., Fuentes J., Gaïti C., Gallais P., Kajfasz E., Langarica R., Langlois A., Larrieu M., Le Van Suu A., Lecubin J., López Ángeles E., Lugo E., Malgoyre A., Mathon R., Moreau C., Nouvel-De-La-Flèche A., Ochoa J.L., Pedrayes-López M., Ramon P., Ruíz-Díaz-Soto J., Tinoco S., Valentin H.

Publicada: 1 ene 2022
Resumen:
Cosmic explosions have emerged as a major field of astrophysics over the last years with our increasing capability to monitor large parts of the sky in different wavelengths and with different messengers (photons, neutrinos, and gravitational waves). In this context, gamma-ray bursts (GRBs) play a very specific role, as they are the most energetic explosions in the Universe. The forthcoming Sino-French SVOM mission will make a major contribution to this scientific domain by improving our understanding of the GRB phenomenon and by allowing their use to understand the infancy of the Universe. In order to fulfill all of its scientific objectives, SVOM will be complemented by a fast robotic 1.3 m telescope, COLIBRI, with multiband photometric capabilities (from visible to infrared). This telescope is being jointly developed by France and Mexico. The telescope and one of its instruments are currently being extensively tested at OHP in France and will be installed in Mexico in spring 2023. © 2022 SPIE.

Filiaciones:
Basa S.:
 Aix-Marseille University, Cnrs, Cnes, Lam, Marseille, France

Lee W.H.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Dolon F.:
 Aix-Marseille University, Cnrs, Ohp, France

Watson A.M.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Floriot J.:
 Aix-Marseille University, Cnrs, Cnes, Lam, Marseille, France

Atteia J.-L.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Butler N.R.:
 Arizona State University, United States

Dornic D.:
 Aix-Marseille University, CNRS/IN2P3, Cppm, IPhU, Marseille, France

Lombardo S.:
 Aix-Marseille University, Cnrs, Cnes, Lam, Marseille, France

Ronayette S.:
 Aix-Marseille University, Cnrs, OSU-Pytheas, France

Ageron M.:
 Aix-Marseille University, CNRS/IN2P3, Cppm, IPhU, Marseille, France

Agneray F.:
 Aix-Marseille University, Cnrs, Cnes, Lam, Marseille, France

Ángeles F.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Bautista L.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Benamar-Aissa H.:
 Aix-Marseille University, CNRS/IN2P3, Cppm, IPhU, Marseille, France

Blanpain C.:
 Université Paris-Saclay, Cea, Cnrs, Aim, Gif-sur-Yvette, F-91191, France

Boulade O.:
 Aix-Marseille University, Cnrs, OSU-Pytheas, France

Boy J.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Buat V.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Cadena E.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Cuevas S.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Farah A.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Figueroa L.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Fuentes J.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Gaïti C.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Gallais P.:
 Aix-Marseille University, Cnrs, OSU-Pytheas, France

Kajfasz E.:
 Aix-Marseille University, CNRS/IN2P3, Cppm, IPhU, Marseille, France

Langarica R.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Langlois A.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Larrieu M.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Le Van Suu A.:
 Aix-Marseille University, Cnrs, Ohp, France

Lecubin J.:
 Université Paris-Saclay, Cea, Cnrs, Aim, Gif-sur-Yvette, F-91191, France

López Ángeles E.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Lugo E.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Malgoyre A.:
 Université Paris-Saclay, Cea, Cnrs, Aim, Gif-sur-Yvette, F-91191, France

Mathon R.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Moreau C.:
 Aix-Marseille University, Cnrs, Cnes, Lam, Marseille, France

Nouvel-De-La-Flèche A.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Ochoa J.L.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Pedrayes-López M.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Ramon P.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France

Ruíz-Díaz-Soto J.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Tinoco S.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Cd Universitaria, Apdo. Postal 70-264, Mexico

Valentin H.:
 Irap, Université de Toulouse, Cnrs, Cnes, Ups, France
ISSN: 0277786X
Editorial
SPIE-INT SOC OPTICAL ENGINEERING, 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA, Estados Unidos America
Tipo de documento: Conference Paper
Volumen: 12182 Número:
Páginas:
WOS Id: 000865326800046

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