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ECLAIRs: the SVOM high-energy transient trigger camera

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Godet, O., Atteia, J. -L., Schanne, S., Lachaud, C., Goldwurm, A., Piron, F., Guillemot, Ph., Amoros, C., Bertoli, W., Bouchet, L., Charmeau, M. C., Chteau, F., Cordier, B., Dagoneau, N., Daly, F., Dezalay, J. -P., Galezzi, J., Givaudan, A., Gros, A., Karakac, M., Lacombe, K., Leprovost, H., Maestre, S., Mercier, K., Pasquier, H., Perraud, L., Pons, R., Rambaud, D., Simonella, O., Tourrette, T., Triou, H., Waegebaert, V., Bacon, P., Barlyaeva, T., Bellemont, N., Bernardini, M. -G., Brunet, M., Cangemi, F., Cavet, C., Coleiro, A., Corre, D., Daigne, F., Foisseau, A., Gevin, O., Guillot, S., Jacob, U., Lacreu, F., Stum, S. Le, Maeght, P., Maiolino, T., Maolo, A., Tcherniatinksy, G., Wang, J., Yang, H.
Natura:	Preprint
Pubblicazione:	2026
Soggetti:	High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
Accesso online:	Acceder al recurso
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author	Godet, O. Atteia, J. -L. Schanne, S. Lachaud, C. Goldwurm, A. Piron, F. Guillemot, Ph. Amoros, C. Bertoli, W. Bouchet, L. Charmeau, M. C. Chteau, F. Cordier, B. Dagoneau, N. Daly, F. Dezalay, J. -P. Galezzi, J. Givaudan, A. Gros, A. Karakac, M. Lacombe, K. Leprovost, H. Maestre, S. Mercier, K. Pasquier, H. Perraud, L. Pons, R. Rambaud, D. Simonella, O. Tourrette, T. Triou, H. Waegebaert, V. Bacon, P. Barlyaeva, T. Bellemont, N. Bernardini, M. -G. Brunet, M. Cangemi, F. Cavet, C. Coleiro, A. Corre, D. Daigne, F. Foisseau, A. Gevin, O. Guillot, S. Jacob, U. Lacreu, F. Stum, S. Le Maeght, P. Maiolino, T. Maolo, A. Tcherniatinksy, G. Wang, J. Yang, H.
author_facet	Godet, O. Atteia, J. -L. Schanne, S. Lachaud, C. Goldwurm, A. Piron, F. Guillemot, Ph. Amoros, C. Bertoli, W. Bouchet, L. Charmeau, M. C. Chteau, F. Cordier, B. Dagoneau, N. Daly, F. Dezalay, J. -P. Galezzi, J. Givaudan, A. Gros, A. Karakac, M. Lacombe, K. Leprovost, H. Maestre, S. Mercier, K. Pasquier, H. Perraud, L. Pons, R. Rambaud, D. Simonella, O. Tourrette, T. Triou, H. Waegebaert, V. Bacon, P. Barlyaeva, T. Bellemont, N. Bernardini, M. -G. Brunet, M. Cangemi, F. Cavet, C. Coleiro, A. Corre, D. Daigne, F. Foisseau, A. Gevin, O. Guillot, S. Jacob, U. Lacreu, F. Stum, S. Le Maeght, P. Maiolino, T. Maolo, A. Tcherniatinksy, G. Wang, J. Yang, H.
contents	The core instrument of the SVOM Gamma-ray burst mission launched in June 2024 is the 4-150 keV 2-D coded mask camera ECLAIRs responsible for the autonomous trigger and localization of transient events within its field of view. The flight model of ECLAIRs has been built by several French labs (IRAP, CEA, APC) under the supervision of the French Space Agency (CNES), while APC, LUPM and IAP built a suite of data reduction and analysis software. This paper outlines the main science goals of ECLAIRs and describes the different instrument sub-systems and their main characteristics. The paper then discusses the instrument configuration and operation as well as the main in-flight measured performances. Finally, the paper summarizes the science performance of ECLAIRs up to March 31, 2025.
format	Preprint
id	arxiv_https___arxiv_org_abs_2604_24249
institution	arXiv
publishDate	2026
record_format	arxiv
spellingShingle	ECLAIRs: the SVOM high-energy transient trigger camera Godet, O. Atteia, J. -L. Schanne, S. Lachaud, C. Goldwurm, A. Piron, F. Guillemot, Ph. Amoros, C. Bertoli, W. Bouchet, L. Charmeau, M. C. Chteau, F. Cordier, B. Dagoneau, N. Daly, F. Dezalay, J. -P. Galezzi, J. Givaudan, A. Gros, A. Karakac, M. Lacombe, K. Leprovost, H. Maestre, S. Mercier, K. Pasquier, H. Perraud, L. Pons, R. Rambaud, D. Simonella, O. Tourrette, T. Triou, H. Waegebaert, V. Bacon, P. Barlyaeva, T. Bellemont, N. Bernardini, M. -G. Brunet, M. Cangemi, F. Cavet, C. Coleiro, A. Corre, D. Daigne, F. Foisseau, A. Gevin, O. Guillot, S. Jacob, U. Lacreu, F. Stum, S. Le Maeght, P. Maiolino, T. Maolo, A. Tcherniatinksy, G. Wang, J. Yang, H. High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics The core instrument of the SVOM Gamma-ray burst mission launched in June 2024 is the 4-150 keV 2-D coded mask camera ECLAIRs responsible for the autonomous trigger and localization of transient events within its field of view. The flight model of ECLAIRs has been built by several French labs (IRAP, CEA, APC) under the supervision of the French Space Agency (CNES), while APC, LUPM and IAP built a suite of data reduction and analysis software. This paper outlines the main science goals of ECLAIRs and describes the different instrument sub-systems and their main characteristics. The paper then discusses the instrument configuration and operation as well as the main in-flight measured performances. Finally, the paper summarizes the science performance of ECLAIRs up to March 31, 2025.
title	ECLAIRs: the SVOM high-energy transient trigger camera
topic	High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
url	https://arxiv.org/abs/2604.24249