arXiv · astro-ph/9712285
BeppoSAX observations of PKS 0528+134
Abstract
We report on the BeppoSAX observations of the gamma-ray blazar PKS 0528+134 performed in Feb and Mar 1997, during a multiwavelength campaign involving EGRET and ground based telescopes. The source was in a faint and hard state, with energy spectral index alpha=0.48+-0.04 between 0.1 and 10 keV, and [2-10] keV flux of 2.7E-12 erg/cm2/s. No significant variability was observed. The source was detected in the 20-120 keV band by the PDS, with a flux lying slightly above the extrapolation from lower X-ray energies. Comparing this low state with previous higher states of the source, there is an indication that the X-ray spectrum hardens and the gamma-ray spectrum steepens when the source is fainter.
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G. Ghisellini, G. Tagliaferri, L. Costamante, L. Maraschi, A. Celotti, G. Fossati, L. Bassani, M. Cappi, F. Frontera, E. Pian, A. Comastri, M. Cavallone, G. De Francesco, L. Lanteri, C. M. Raiteri, G. Sobrito, M. Villata, S. Giarrusso, B. Sacco, I. S. Glass, P. Grandi, E. Massaro, S. Molendi, P. Padovani, G. G. C. Palumbo, C. Perola, M. Salvati, A. Treves. 1997-12-21. BeppoSAX observations of PKS 0528+134. https://doi.org/10.1016/s0920-5632(98)00255-2
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