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Precise GRB source locations from the renewed interplanetary network
DOI: 10.1051/aas:1999350 Bibcode: 1999A&AS..138..557C

Hurley, K.; Kouveliotou, C.; Cline, T. L. +14 more

A new interplanetary network (IPN) is made possible by the modification of the NEAR mission, now at 2 AU distance. With Ulysses and the near-Earth GRB monitors, this fully long-baseline network will produce GRB localizations at a rate of about one per week, with accuracies varying from several to tens of arc minutes. Given the delays inherent in t…

1999 Astronomy and Astrophysics Supplement Series
Ulysses 10
The peak flux distribution of bright gamma-ray bursts measured with ULYSSES
DOI: 10.1051/aas:1999292 Bibcode: 1999A&AS..138..421A

Hurley, K.; Atteia, J. -L.; Boër, M.

Observations of gamma-ray burst afterglows have shown that these events come from formidable explosions at cosmological distances. If the most distant GRBs seen by BATSE have redshifts of the order of 3-6 (e.g. GB 971214), it is a coincidence that the bright end of the GRB intensity distribution displays the -3/2 slope expected for a Euclidean dis…

1999 Astronomy and Astrophysics Supplement Series
Ulysses 5