Abstract
Radio observations may be one of the most promising but least explored bands of the spectrum to search for the counterparts of gamma ray bursters. We describe several ongoing experiments with demonstrated high sensitivity to monitor gamma ray bursts for evidence of a flaring or fading counterpart in the days, weeks and months following the original event.
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References
Cline, T. L. et al.: 1994, in Gamma Ray Bursts, Second Workshop, eds. G. J. Fishman, J. J. Brainerd, K. Hurley (American Institute of Physics: New York), p. 373.
Frail, D. A.et al.: 1994, Astrophys. J.,437, L43.
Hanlon, L. O.,et al.: 1995, these proceedings.
Hurley, K. C.,et al.: 1995, these proceedings.
Katz, J. I.: 1994, Astrophys. J.,432, L107.
Koranyi, D. M.,et al.: 1994, MNRAS,271, 51.
McNamara, B.,et al.: 1995, these proceedings.
Meszaros, P. and Rees, M. J.: 1993, Astrophys. J.,405, 278.
Paczyński, B. and Rhoads, J. E.: 1993, Astrophys. J.,418, L5.
Palmer, D. M.,et al.: 1995, these proceedings.
Ricker, G. R.et al.: 1995, these proceedings.
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Frail, D.A., Kulkarni, S.R. Radio counterpart searches of gamma ray bursts. Astrophys Space Sci 231, 277–280 (1995). https://doi.org/10.1007/BF00658631
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DOI: https://doi.org/10.1007/BF00658631