GRB Repetition Limits from Current BATSE Observations

(2) NASA/MSFC; (3) University of Alabama in Huntsville; (4) Clemson University; (5) National Research Council at NASA/MSFC); Charles A. Meegan (2); Dieter H. Hartmann (4); Geoffrey N. Pendleton (3); John M. Horack (2); Jon Hakkila (1); Michael S. Briggs (3)

arxiv: astro-ph/9712092 · v1 · submitted 1997-12-05 · 🌌 astro-ph

GRB Repetition Limits from Current BATSE Observations

Jon Hakkila (1) , Charles A. Meegan (2) , Geoffrey N. Pendleton (3) , Michael S. Briggs (3) , John M. Horack (2) , Dieter H. Hartmann (4) , Valerie Connaughton (5) ((1) Mankato State University , (2) NASA/MSFC

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(3) University of Alabama in Huntsville (4) Clemson University (5) National Research Council at NASA/MSFC)

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keywords batserepetitionburstlimitsassumedburstscatalogscurrent

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Revised upper limits on gamma-ray burst repetition rates are found using the BATSE 3B and 4B catalogs. A statistical repetition model is assumed in which sources burst at a mean rate but in which BATSE observes bursts randomly from each source.

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GRB Repetition Limits from Current BATSE Observations

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