Fig. 6 from A Search for TeV Counterparts to BATSE Gamma‐Ray Bursts

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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. 6.

BATSE spectra for 1995 May 24, 1995 July 1, and 1995 December 20 bursts (Band model) extended to 1 TeV. The upper limit at 0.3 TeV is the Whipple result for a source at the center of the camera in position A of each set of observations. The dashed line is an extrapolation of the BATSE spectrum, which is calculated from photons of energy of approximately 30–1800 keV.

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