Precise GRB source locations from the renewed interplanetary network

被引：10

作者：

Cline, TL ^{[1
]}

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

Meegan, C

机构：

[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[3] APL, Laurel, MD 20723 USA

[4] AF Ioffe Phys Tech Inst, St Petersburg 194021, Russia

[5] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 138卷 / 03期

关键词：

gamma-rays : bursts; instrumentation : miscellaneous;

D O I：

10.1051/aas:1999350

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 are 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.

引用

页码：557 / 558

页数：2