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Table 1.

Confirmed quasar pairs. We show the separation between the two images from Gaia, the spectroscopic redshift, and the Gaia G magnitudes.

Object RA Dec Gaia (PSF) Sep. Gaia G-mag z Type Referenced by
PS J0125−1012 21.3174 −10.2082 1.12″ (1.13″) 19.25, 20.61 1.22 UQP Lemon et al. (2023)
PS J0240−0208 40.0768 −2.1474 0.94″ 18.70, 19.58 1.688, 1.08 Projected pair
PS J0557−2959 89.3979 −29.9933 0.81″ (0.80″) 19.50, 20.56 2.04 Lens
PS J0909−0749 137.4946 −7.8179 0.81″ (0.82″) 18.25, 19.05 1.08 UQP
PS J1019−1322 154.8066 −13.3692 1.13″ (1.13″) 19.57, 20.41 2.32 UQP
PS J1037+0018 159.3665 0.3057 1.24″ (1.23″) 18.05, 19.99 2.46 Lens
PS J1225+4831 186.3278 48.5212 0.90″ 18.00, 19.26 3.09 UQP Yue et al. (2023)
PS J1800+0146 270.0320 1.7767 1.12″ (1.12″) 18.39, 18.72 1.53 Lens
PS J2122−1621 320.6075 −16.357 1.20″ (1.21″) 19.14, 19.26 1.47 Lens

Notes. When applicable, we also indicate the separation recovered from the models in Figs. 2 and 5.

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