The InterPlanetary Network Supplement to the Second Fermi GBM Catalog of Cosmic Gamma-Ray Bursts

InterPlanetary Network (IPN) data are presented for the gamma-ray bursts in the second Fermi Gamma-Ray Burst Monitor (GBM) catalog. Of the 462 bursts in that catalog between 2010 July 12 and 2012 July 11, 428, or 93%, were observed by at least 1 other instrument in the 9-spacecraft IPN. Of the 428,...

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Veröffentlicht in:The Astrophysical journal. Supplement series 2017-04, Vol.229 (2), p.31-31
Hauptverfasser: Hurley, K., Aptekar, R. L., Golenetskii, S. V., Frederiks, D. D., Svinkin, D. S., Pal'shin, V. D., Briggs, M. S., Meegan, C., Connaughton, V., Goldsten, J., Boynton, W., Fellows, C., Harshman, K., Mitrofanov, I. G., Golovin, D. V., Kozyrev, A. S., Litvak, M. L., Sanin, A. B., Rau, A., Kienlin, A. von, Zhang, X., Yamaoka, K., Fukazawa, Y., Ohno, M., Tashiro, M., Terada, Y., Barthelmy, S., Cline, T., Gehrels, N., Cummings, J., Krimm, H. A., Smith, D. M., Monte, E. Del, Feroci, M., Marisaldi, M.
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Sprache:eng
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Zusammenfassung:InterPlanetary Network (IPN) data are presented for the gamma-ray bursts in the second Fermi Gamma-Ray Burst Monitor (GBM) catalog. Of the 462 bursts in that catalog between 2010 July 12 and 2012 July 11, 428, or 93%, were observed by at least 1 other instrument in the 9-spacecraft IPN. Of the 428, the localizations of 165 could be improved by triangulation. For these bursts, triangulation gives one or more annuli whose half-widths vary between about 2 3° and 16°, depending on the peak flux, fluence, time history, arrival direction, and the distance between the spacecraft. We compare the IPN localizations with the GBM 1 , 2 , and 3 error contours and find good agreement between them. The IPN 3 error boxes have areas between about 8 square arcminutes and 380 square degrees, and are an average of 2500 times smaller than the corresponding GBM 3 localizations. We identify four bursts in the IPN/GBM sample whose origins were given as "uncertain," but may in fact be cosmic. This leads to an estimate of over 99% completeness for the GBM catalog.
ISSN:0067-0049
1538-4365
DOI:10.3847/1538-4365/229/2/31