  The novel Gaia Multi Peak (GMP) technique has proven to be able to
successfully select dual and lensed AGN candidates at sub-arcsec separations.
Both populations are important because dual AGNs represent one of the central,
still largely untested, predictions of lamdaCDM cosmology, and compact lensed
quasars allow to probe the central regions of the lensing galaxies. In this
work, we present high spatial resolution spectroscopy of twelve GMP-selected
systems. We use the the adaptive-optics assisted integral-field spectrograph
MUSE at VLT to resolve each system and study the nature of each component. All
the targets reveal the presence of two components confirming the GMP selection.
We classify five targets as dual AGNs, two as lensed systems, and five as a
chance alignment of a star and and AGN. Having separations between 0.30" and
0.86", these dual and lensed systems are, to date, among the most compact ever
discovered at z >0.3. This is the largest sample of distant dual AGNs with
sub-arcsec separations ever presented in a single paper.

Astrophysics of Galaxies