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Simple expressions for the radius and magnetic field of a system emitting synchrotron self‐absorbed radio and inverse‐Compton X‐rays are derived from first principles which involve observable quantities only. These expressions are useful for analysing observations of supernova blast waves interacting with dense circumstellar material at early times.

Radius and magnetic field from synchrotron self‐absorbed radio and inverse‐Compton X‐ray observations of supernovae