10$ and $t_\mathrm{d}$ in units of days. The parameters used here are specified in Table \[tab:wsedp\].

  --------------------------------------------- --------------------- ---------------------
  SSC model input                               Low state             Flare SED
  parameter                                     SED (MAGIC)           
  Doppler factor $\delta$                       8.4                   15.2
  Magnetic field strength $B$                   0.095 G               0.075 G
  Emission region radius $R$                    $10^{16}$ cm          $10^{16}$ cm
  Electron density $\rho$                       0.025 erg cm$^{-3}$   0.025 erg cm$^{-3}$
  ${E_{\mathrm{min}}} [\log E({\rm eV})]$       9.1                   8.9
  ${E_{\mathrm{max}}} [\log E({\rm eV})]$       11.6                  11.9
  ${E_{\mathrm{br}}} [\log E({\rm eV})]$        10.9                  10.9
  $n(E_\mathrm{min}<E\leq {E_{\mathrm{br}}})$   -2.2                  -2.2
  $n(E_\mathrm{br}<E\leq {E_{\mathrm{max}}})$   -3.2                  -3.2
  --------------------------------------------- --------------------- ---------------------

  : Model input parameters used with the SSC model provided by @Krawczynski1es1959-2004 for describing the MAGIC low emission state and the 1995 Whipple flare emission state as depicted in Fig. \[fig:wsed\].[]{data-label="tab:wsedp"}

The two models shown are to represent both the flare state of 1995 and the MAGIC observations in 2005. They differ in the following model input parameters: (1) in the Doppler factor, (2) in the magnetic field strength, and (3) the minimum and maximum electron energy. In addition, the form of the electron spectrum differs for the two flux states. The radius of the emission region was kept constant at $10^{14}$ m. While most of the model parameters are compatible with 