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A Search for TeV Counterparts to BATSE Gamma‐Ray Bursts

  • Authors: V. Connaughton, C. W. Ackerlof, S. Barthelmy, S. Biller, P. Boyle, J. Buckley, D. A. Carter-Lewis, M. Cantanese, M. F. Cawley, T. Cline, D. J. Fegan, J. Finley, G. J. Fishman, J. Gaidos, N. Gehrels, A. M. Hillas, C. Kouveliotou, F. Krennrich, R. C. Lamb, R. Lessard, J. McEnery, C. Meegan, G. Mohanty, N. A. Porter, J. Quinn, A. Rodgers, H. J. Rose, F. Samuelson, M. S. Schubnell, G. Sembroski, R. Srinivasan, T. C. Weekes, C. Wilson, and J. Zweerink

Connaughton et al. 1997 The Astrophysical Journal 479 859.

  • Provider: AAS Journals

Caption: Fig. 1.

Response to BACODINE notification. Each circle represents the field of view of the 10 m reflector at different positions following a BATSE burst. The numbers in the circles indicate the sequence of observations. The centers of the circles are 3° apart, and the center of the first observation is at the coordinates given for the BATSE burst. There is some overlap between the observations, since the instrument is sensitive to showers from sources outside the geometrical field of view. A typical BATSE location error box is also shown.

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