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Multiwavelength observations are now the norm for studying blazars' variousstates of activity, classifying them, and determining possible underlyingphysical processes driving their emission. Broadband emission models becameunavoidable tools for testing emission scenarios and setting values to physicalquantities such as the magnetic field strength, Doppler factor, or shape of theparticle distribution of the emission zone(s). We announce here the firstpublic release of a new tool, Bjet_MCMC, that can automatically fit broadbandspectral energy distributions (SEDs) of blazars. The complete code is availableon GitHub and allows testing leptonic synchrotron self-Compton models (SSC),with or without external inverse-Compton processes from the thermal environmentof supermassive black holes (accretion disk and broad line region). The code isdesigned to be user-friendly and computationally efficient. It contains a corewritten in C++ and a fully parallelized SED fitting method. The originalmulti-SSC zones model of Bjet is also available on GitHub but is not includedin the MCMC fitting process at the moment. We present the features,performance, and results of Bjet_MCMC, as well as user advice.

Bjet_MCMC: A new tool to automatically fit the broadband SEDs of blazars