Abstract
Abstract We report the discovery of a close quasar pair candidate at z = 5.66, J2037–4537. J2037–4537 is resolved into two quasar images at the same redshift in ground-based observations. Follow-up spectroscopy shows significant differences in both the continuum slopes and emission line properties of the two images. The two quasar images have a projected separation of 1.″24 (7.3 kpc at z = 5.66) and a redshift difference of Δz ≲ 0.01. High-resolution images taken by the Hubble Space Telescope do not detect the foreground lensing galaxy. The observational features of J2037–4537 strongly disfavor the lensing hypothesis. If J2037–4537 is a physical quasar pair, it indicates a quasar clustering signal of ∼105 at a separation of ∼10 proper kpc (pkpc), and gives the first observational constraint on the pair fraction of z > 5 quasars, f pair(r < 30 pkpc) > 0.3%. The properties of J2037–4537 are consistent with those of merger-triggered quasar pairs in hydrodynamical simulations of galaxy mergers.
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