The faint voice of a radio-weak BL Lacertae: modeling the broadband emission of WISE J141046.00+740511.2

The WISE source, J141046.00+740511.2, has been recently observed from radio to γ rays. Although the optical spectrum is consistent with a BL Lacertae (BL Lac) object, the source displays unusually weak radio emission, which challenges standard interpretations. Our aim is to understand the origin of the broadband emission from J141046.00+740511.2, using a leptonic model of an extended jet. To obtain the distribution of electrons along the conical jet, we solved a steady-state convective transport