arXiv · astro-ph/9902224
Correlated variability of Mkn 421 at X-ray and TeV wavelengths on timescales of hours
Abstract
Mkn 421 was observed for about two days with BeppoSAX, prior to and partly overlapping the start of a 1 week continuous exposure with ASCA in April 1998, as part of a world-wide multiwavelength campaign. A pronounced, well defined, flare observed in X-rays was also observed simultaneously at TeV energies by the Whipple Observatory's 10 m gamma-ray telescope. These data provide the first evidence that the X-ray and TeV intensities are well correlated on time-scales of hours.
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L. Maraschi, G. Fossati, F. Tavecchio, L. Chiappetti, A. Celotti, G. Ghisellini, P. Grandi, E. Pian, G. Tagliaferri, A. Treves, A. C. Breslin, J. H. Buckley, D. A. Carter-Lewis, M. Catanese, M. F. Cawley, D. J. Fegan, S. Fegan, J. Finley, J. Gaidos, T. Hall, A. M. Hillas, F. Krennrich, R. W. Lessard, C. Masterson, P. Moriarty, J. Quinn, J. Rose, F. Samuelson, T. C. Weekes. 1999-02-16. Correlated variability of Mkn 421 at X-ray and TeV wavelengths on timescales of hours. https://doi.org/10.1016/s0927-6505(99)00046-8
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