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Solve the following problem using Python, implementing the functions described below, one line at a time
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Description:
 def ElectronIC(pars, data):
 """ Define particle distribution model, radiative model, and return model flux at data energy values """


    ECPL = ExponentialCutoffPowerLaw(
        pars[0] / u.eV, 10.0 * u.TeV, pars[1], 10 ** pars[2] * u.TeV
    )
    IC = InverseCompton(ECPL, seed_photon_fields=["CMB"])

    return IC.flux(data, distance=1.0 * u.kpc)