  By discovering a narrow-line emitter embedded in an extended Ly-alpha nebula,
Husemann et al. (2018) found that the luminous radio-quiet quasar LBQS
0302-0019 is a dual active galactic nucleus (AGN) system. By combining
available archival radio interferometric data taken at 8.4 GHz with the Very
Large Array (VLA), we found that the weak 0.4-mJy radio source in this system
positionally coincides with the unobscured optical quasar while its newly
discovered obscured companion has no detectable radio emission (<0.045
mJy/beam, 3-sigma image noise level). However, the non-detection of this object
with the VLA does not rule out the presence of a radio-quiet AGN there.
