  Merger events can trigger gas accretion onto supermassive black holes (SMBHs)
sitting at the centre of galaxies, and form close pairs of active galactic
nuclei (AGN). The fraction of AGN in pairs gives key information to constrain
the environmental properties and evolution of SMBHs and their host galaxies.
However, the identification of dual AGN is difficult, and only very few have
been found in the distant Universe so far. We report the serendipitous
discovery of a triple AGN and four dual AGN (one considered as a candidate),
with projected separations in the range 3-28 kpc. Their AGN classification is
mostly based on classical optical emission line flux ratios, as observed with
the Near-InfraRed Spectrograph (NIRSpec) on the James Webb Space Telescope
(JWST), and is complemented with additional multi-wavelength diagnostics. The
identification of these multiple AGN out of the 17 AGN systems in our GA-NIFS
survey (i.e. ~ 20-30%), suggests that they might be more common than expected
from the most recent cosmological simulations, which predict a fraction of dual
AGN at least one order of magnitude smaller. This work highlights the
exceptional capabilities of NIRSpec for detecting distant dual AGN, and prompts
new investigations to better constrain their fraction across the cosmic time,
and to inform upcoming cosmological simulations.
