A Joint Chandra, Fermi, MAGIC, and VERITAS Broadband Study of One High-Energy Blazar in A Major Outburst

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The main objective of the proposed work is to perform a single very intensive observational campaign at radio, X-ray, GeV, and TeV energies on one of the well-established northern sky TeV blazars, i.e., Mkn 501, 1ES 1959+650, H1426+428, or 1ES 2344+514 with Chandra, Fermi, MAGIC, and VERITAS.During planned multi-wavelength campaign the SED of one blazar will be covered by simultaneous observations with VLBI, Chandra, Fermi, MAGIC, and VERITAS all the way from radio through TeV γ rays. Our scientific goal is to derive ma jor physical parameters of the AGN jet by reproducing the complete SED, using both leptonic and hadronic models, which can infer the bulk Lorentz factor and the total power of the jet.

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