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1999A&AS..138..557C - Astron. Astrophys., Suppl. Ser., 138, 557-558 (1999/September-0)
Precise GRB source locations from the renewed interplanetary network.
CLINE T.L., BARTHELMY S., BUTTERWORTH P., MARSHALL F., McCLANAHAN T., PALMER D., TROMBKA J., HURLEY K., GOLD R., APTEKAR R., FREDERIKS D., GOLENETSKII S., IL'INSKII V., MAZETS E., FISHMAN G., KOUVELIOTOU C. and MEEGAN C.
Abstract (from CDS):
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 the collection of deep space data, high-precision alerts with delays under one day should be possible at a rate of one to several per month. An automatic analysis system is being developed to optimize the process.
Abstract Copyright: ∼
Journal keyword(s): gamma-rays: bursts - instrumentation: miscellaneous
Simbad objects: 1
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