arXiv · astro-ph/9706142
TeV Observations of the Variability and Spectrum of Markarian 501
Abstract
Markarian 501 is only the second extragalactic source to be detected with high statistical certainty at TeV energies; it is similar in many ways to Markarian 421. The Whipple Observatory gamma-ray telescope has been used to observe the AGN Markarian 501 in 1996 and 1997, the years subsequent to its initial detection. The apparent variability on the one-day time-scale observed in TeV gamma rays in 1995 is confirmed and compared with the variability in Markarian 421. Observations at X-ray and optical wavelengths from 1997 are also presented.
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J. Quinn, I. H. Bond, P. J. Boyle, J. H. Buckley, S. M. Bradbury, A. C. Breslin, A. M. Burdett, J. Bussons Gordo, D. A. Carter-Lewis, M. Catanese, M. F. Cawley, D. J. Fegan, J. P. Finley, J. A. Gaidos, A. Hall, A. M. Hillas, F. Krennrich, R. C. Lamb, R. W. Lessard, C. Masterson, J. E. McEnery, G. Mohanty, P. Moriarty, A. J. Rodgers, H. J. Rose, F. W. Samuelson, G. H. Sembroski, R. Srinivasan, T. C. Weeke, J. Zweerink. 1997-06-15. TeV Observations of the Variability and Spectrum of Markarian 501. https://arxiv.org/abs/astro-ph/9706142
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