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Table B.1.

Fast cooling: list of all possible radiative regimes and corresponding electron distribution.

Notes. For each case, the first row of the table gives the list of breaks appearing either in the normalised electron distribution f(x) (i.e. the list of xi), or in the normalised Compton parameter h(x) (i.e. the list of relevant x ^ i $ \widehat{x}_i $), as well as all other necessary characteristic Lorentz factors to fully define the case in agreement with Fig. B.1 (blue). The break corresponding to the peak of the synchrotron spectrum is highlighted in red. The second and third rows give the slopes −dlnf/dlnx and −dlng/dlnx for each branch. Finally, the last column gives the expression of γ0. Cases F24 and F25 require a specific treatment: see text in appendix B.

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