Abstract We perform a systematic search for galactic-scale quasar pairs and small-scale ( 0.5 (803 double quasars out of 2497 pairs without any cuts) with separations of ∼ 0 . ″ 3 – 3 ″ , corresponding to projected physical separations of ∼3–30 kpc at the median redshift z = 1.7 for the sample. Candidate unobscured double quasars are selected as Gaia-resolved pairs around spectroscopically confirmed SDSS quasars ( L bol > 10 44.5 erg s −1 ) at 0.5 5 . 7 − 0.3 + 0.3 × 1 0 − 4 (bootstrapping errors). The double quasar fraction measured in individual separation bins increases toward smaller separations, consistent with earlier findings. The dual quasar fraction also shows little redshift evolution for the luminous SDSS sample, in agreement with previous observations and simulation. However, the observed fraction is lower than simulation predictions by ∼0.8–1.6 dex, suggesting a significant population of obscured quasar pairs are missed in our search. Future wide-area space missions targeting both unobscured and obscured quasar pairs at subarcsecond resolutions will reveal the population of obscured quasar pairs and extend to much lower luminosities of active galactic nuclei.
Jiang et al. (Wed,) studied this question.
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