Observing strategies using GCN

Details Observing strategies using GCN Observing strategies using GCN

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..129b&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 129-133 (1998).

Computer Science

3

Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray, X- And Gamma-Ray Telescopes And Instrumentation, Observation And Data Reduction Techniques, Computer Modeling And Simulation

Scientific paper

Given the broad range of error box sizes available from the GRB Coordinates Network (GCN) and the range of time delays involved, there is now the opportunity for many more instruments, than could use the old BACODINE system, to make follow-up observations to detect the GRB counterpart. We present a set of scenarios (some taken from existing GCN site operations and some from anticipated operations) to guide the potential new observer in matching his/her instrument's capabilities with the GCN burst location information and in setting up the follow-up observing procedures.

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