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The sources SDSS\,J113126.08-020459.2 and SDSS\,J110851.04+065901.4 are twodouble-peaked [O III] emitting AGN, identified as candidate binary AGNs byoptical and near infrared (NIR) observations. We observed the two sources withhigh resolution Very Long Baseline Interferometry (VLBI) using the EuropeanVLBI Network at 5\,GHz, reduced VLA observations at three frequencies availablefor one of the sources, and used archival HST observations.  For the source SDSS\,J113126.08-020459.2, the VLBI observations detected onlyone single compact component associated with the eastern NIR nucleus. InSDSS\,J110851.04+065901.4, the VLBI observations did not detect any compactcomponents, but the VLA observations allowed us to identify a possible compactcore in the region of the north-western optical/NIR nucleus. In this source wefind kpc-scale extended radio emission that is spatially coincident to theultraviolet continuum and to the extended emission narrow line region. The UVcontinuum is significantly obscured since the amount of extended radio emissionyields a star formation rate of about 110 \msunyr, which is an order ofmagnitude larger than implied by the observed ultraviolet emission.  Our analysis confirms the presence of only one AGN in the two candidatebinary AGNs.

Unveiling the radio counterparts of two binary AGN candidates: J1108+0659 and J1131-0204