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Conclusion

Gamma-ray bursts posses a number of properties that make them very good candidates for synchronizers that could aid in the search for brief beamed extraterrestrial signals. GRB positions are now starting to be obtained with sufficient precision to make them useful for targeted searches. This is augmented by precise measurements of stellar parallaxes from satellite borne instruments, and it is anticipated that even better parallax measurements will be obtained in the relatively near future. GRB locations and times are rapidly available from the GCN (GRB Coordinates Network, Barthelmy et al. 1998) and this is likely to continue with future missions which also aids in their use.

For all sky surveys, the case for using GRBs as target positions to observe may be a lot weaker. However, there appears to be little to lose by pointing a detector as soon as possible at GRB locations and monitoring that location for some time. Additionally, even the positions currently provided by BATSE may be used for this purpose by a detector that has a field of view of a few degrees.




 
Table 1: Time Delays between GRB and Transmitted Signal
Distance (pc) Angle($^{\circ}$) Delay (d) 1 10 Hipparcos GAIA/SIM
7.2 1 1.30631 7.25609E-04 7.26718E-03 9.47365E-03 9.40612E-05
7.2 2 5.22485 1.45110E-03 1.45221E-02 3.78917E-02 3.76216E-04
7.2 3 11.7544 2.17615E-03 2.17725E-02 8.52456E-02 8.46379E-04
7.2 5 32.6379 3.62403E-03 3.62514E-02 0.236697 2.35010E-03
20 1 3.62864 2.01558E-03 2.01866E-02 7.40539E-02 7.25874E-04
20 2 14.5135 4.03083E-03 4.03391E-02 0.296193 2.90327E-03
20 3 32.6512 6.04485E-03 6.04793E-02 0.666350 6.53154E-03
20 5 90.6608 1.00668E-02 1.00698E-01 1.85022 1.81358E-02
50 1 9.07161 5.03895E-03 5.04665E-02 0.477453 4.53807E-03
50 2 36.2837 1.00771E-02 1.00848E-01 1.90967 1.81509E-02
50 3 81.6279 1.51121E-02 0.151198 4.29621 4.08344E-02
50 5 226.652 2.51669E-02 0.251746 11.9291 0.113383
100 1 18.1432 1.00779E-02 1.00933E-01 2.01591 1.81614E-02
100 2 72.5673 2.01541E-02 0.201695 8.06304 7.26400E-02
100 3 163.256 3.02242E-02 0.302396 18.1395 0.163419
100 5 453.304 5.03338E-02 0.503491 50.3671 0.453758
1000 1 181.432 1.00779E-01 1.00933 -- 1.83265
1000 2 725.673 0.201541 2.01695 -- 7.33003
1000 3 1632.56 0.302242 3.02396 -- 16.4905
1000 5 4533.04 0.503338 5.03491 -- 45.7883

           
Notes: Time delay and errors are in days. Angle is the offset between the gamma-ray burst and the transmitter. The 1 and 10 columns list the uncertainties due to inaccuracies of 1 and 10 in the position of the GRB respectively. The HIPPARCOS and GAIA/SIM columns give the errors due to uncertainties in the parallax of a transmitter of 1 milli-arcsecond and 10 micro-arcseconds respectively.


next up previous
Next: About this document ... Up: The Use of Gamma-ray Previous: All-sky Signaling
Robin Corbet
1999-06-21