Verifying the accuracy of the third interplanetary network: localization of the bursting pulsar GRO J1744-28 by triangulation

Details Verifying the accuracy of the third interplanetary network: localization of the bursting pulsar GRO J1744-28 by triangulation Verifying the accuracy of the third interplanetary network: localization of the bursting pulsar GRO J1744-28 by triangulation

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998adspr..22.1125h&link_type=abstract

Advances in Space Research, Volume 22, Issue 7, p. 1125-1128.

Physics

Scientific paper

The bursting pulsar GRO J1744-28 is the first repeating source of intense bursts whose position is accurately known, which has become active since the establishment of the third interplanetary network. We show how observations of this object with Ulysses and BATSE can be used to verify many aspects of the triangulation method. Analysis of the preliminary data indicates that there are no unknown sources of error in this method.

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