arXiv · astro-ph/9706132
Search for TeV Counterparts in Gamma-Ray Bursts
Abstract
Based on BACODINE network notification the Whipple Observatory gamma-ray telescope has been used to search for the delayed TeV counterpart to BATSE-detected gamma-ray bursts. In the fast slew mode, any point in the sky can be reached within two minutes of the burst notification. The search strategy, necessary because of the uncertainty in burst position and limited FOV of the camera, is described.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
P. J. Boyle, J. H. Buckley, A. M. Burdett, J. Bussons Gordo, D. A. Carter-Lewis, M. Catanese, M. F. Cawley, V. Connaughton, D. J. Fegan, J. P. Finley, J. A. Gaidos, K. Harris, A. M. Hillas, R. C. Lamb, F. Krennrich, R. W. Lessard, C. Masterson, J. E. McEnery, G. Mohanty, N. A. Porter, J. Quinn, A. J. Rodgers, H. J. Rose, F. W. Samuelson, G. H. Sembroski, R. Srinivasan, T. C. Weekes, J. Zweerink. 1997-06-13. Search for TeV Counterparts in Gamma-Ray Bursts. https://arxiv.org/abs/astro-ph/9706132
Cite the original work for its findings. Save a collection to share your selection of sources.