GRB 031026 (=H2882): evidence for high redshift from prompt.

Atteia, J.-L.; Ricker, G.; Hurley, K.; Jernigan, J. G.; Kawai, N.; Lamb, D.; Woosley, S.; Barraud, C.; Boer, M.; Olive, J.-F.; Dezalay, J.-P.; Donaghy, T.; Graziani, C.; Fenimore, E.; Galassi, M.; Matsuoka, M.; Sakamoto, T.; Shirasaki, Y.; Suzuki, M.; Tamagawa, T.; Torii, K.; Yoshida, A.; Nakagawa, Y.; Satoh, R.; Urata, Y.; Yamazaki, T.; Yamamoto, Y.; Villasenor, J.; Butler, N.; Crew, G.; Doty, J.; Dullighan, A.; Prigozhin, G.; Vanderspek, R.; Azzibrouck, G.; Braga, J.; Manchanda, R.; Pizzichini, G.

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GRB 031026 (=H2882): evidence for high redshift from prompt.

Published in 2003 by J.-L. Atteia, G. Ricker, K. Hurley, J. G. Jernigan, N. Kawai, D. Lamb, S. Woosley, C. Barraud, M. Boer, J.-F. Olive, J.-P. Dezalay, T. Donaghy, C. Graziani, E. Fenimore, M. Galassi and other authors.

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