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The spectral energy distribution (SED) of blazars is generally understoodthrough the standard one-zone synchrotron self-Compton (SSC) model, where astrong correlation between X-ray and TeV gamma-ray fluxes is expected.Recently, for Mrk 421 the correlation was confirmed and interpreted within theSSC model arguing that a description of the correlation up to large flux valuesconsiderably restricts the value of the magnetic field under the assumption ofan electron spectral index independent of the flux state. In this work, weextend the analysis done on Mrk 421 for other two high-energy peaked BL Lacs:Mrk 501 and 1ES 1959+650.

On the TeV gamma-ray and X-ray correlations exhibited in high-energy peaked BL Lacs: Mrk 501 and 1ES 1959+650