X/γ-ray measurements of the faint GRB 020321

Bibcode
2004ASPC..312..209I
in't Zand, J. J. M.; Kuiper, L.; Heise, J.; Amati, L.; Costa, E.; Feroci, M.; Frontera, F.; Gandolfi, G.; Nicastro, L.; Piro, L.; Rodriguez-Pascual, P.; Santos-Lleo, M.; Schartel, N.
Referencia bibliográfica

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference held 17-20 September 2002, in Rome, Italy. Edited by M. Feroci, F. Frontera, N. Masetti, and L. Piro. San Francisco: Astronomical Society of the Pacific, 2004., p.209

Fecha de publicación:
6
2004
Número de autores
13
Número de autores del IAC
0
Número de citas
3
Número de citas referidas
3
Descripción
GRB 020321 is a faint GRB that received wide follow-up attention in X-rays (BeppoSAX/NFI, Chandra/ACIS-S, XMM-Newton), radio (ATCA) and optical (ESO, HST). We identify a weak X-ray afterglow by a combined study of the Chandra and XMM-Newton observations. Its decay index of 1.2 is typical for GRB afterglows. Inside the 4 arcsec accurate error box there is a weak optical counterpart candidate with a much shallower decay index.
Tipo
Sin árbitro

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