VODKA-JWST: Synchronized growth of two SMBHs in a massive gas disk? A 3.8 kpc separation dual quasar at cosmic noon with JWST NIRSpec IFU

The search for dual supermassive black holes (SMBHs) is of immense interest in modern astrophysics. Galaxy mergers may be an important route to fuel and to produce SMBH pairs. Actively accreting SMBH pairs can be observed as a dual quasar, which are vital probes of SMBH growth. Gaia observations have enabled a novel technique to systematically search for such dual quasars at previously unreachable sub-kpc scales, based on the small jitters of the light centroid as the two quasars vary stochastically. Here we present the first detailed study of a 0.46”, 3.8 kpc separation, VODKA-selected dual quasar, J0749+2255, at z=2.17 using JWST/NIRSpec integral field unit spectroscopy. This is one of the most distant, small separation dual quasars identified today. Dual quasars at cosmic noon are not well characterized. We detect the faint ionized gas of the host galaxy, best traced by the narrow emission. Line ratio diagnostics show a mix of ionization from the two quasars and intense star formation. The spatially-resolved spectra of the two quasars suggest that they have very similar black hole properties (two M_BH∼ 10^9M_⊙ with large Eddington ratio reaching L/L_Edd∼0.2) hinting at the possible synchronized growth and accretion from the same gas supply. Surprisingly, the ionized gas kinematics suggest an extended, rotating disk rather than a disturbed system that would be expected in a major gas-rich galaxy merger. While it is unclear if J0749+2255 is representative of the dual quasar evolution, the observations with JWST revealed a major puzzle. It would be interesting to see what observations of other dual quasars will show.