High-resolution MUSE observations of 30 Gaia multipeak targets confirm 19 AGN multiplets including 6 dual AGN, accounting for 22% of known close pairs below 7 kpc and showing the selection method's efficiency.
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Analysis of 204 lensed quasars yields mean source crossing time of 2.59 years, Einstein radius crossing time of 11.29 years, average quasar half-light radius of 5.4 light-days, microlens mass fraction lower limit of 0.15, and 9% probability of high-magnification events.
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Cosmic Duets I. High-spatial resolution spectroscopy of dual and lensed AGN with MUSE-NFM
High-resolution MUSE observations of 30 Gaia multipeak targets confirm 19 AGN multiplets including 6 dual AGN, accounting for 22% of known close pairs below 7 kpc and showing the selection method's efficiency.
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Microlensing time-scales and flux magnification probabilities of a sample of 204 lensed quasars
Analysis of 204 lensed quasars yields mean source crossing time of 2.59 years, Einstein radius crossing time of 11.29 years, average quasar half-light radius of 5.4 light-days, microlens mass fraction lower limit of 0.15, and 9% probability of high-magnification events.