SHARP is positioned to deliver the first statistical census of ultra-compact dual AGN, bridging kpc-scale pairs to sub-pc binary MBHs that emit gravitational waves.
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3 Pith papers cite this work. Polarity classification is still indexing.
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2026 3representative citing papers
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.
Spectroscopic follow-up of 11 candidates from the MGQPC catalog confirms 6 dual quasars and 3 projected quasars, with discussion of prior survey misses and future strategies.
citing papers explorer
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A new era for Dual AGN science with SHARP
SHARP is positioned to deliver the first statistical census of ultra-compact dual AGN, bridging kpc-scale pairs to sub-pc binary MBHs that emit gravitational waves.
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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.
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Search for Quasar Pairs with ${\it Gaia}$ Astrometric Data. III. Discovery of 9 dual and projected quasars
Spectroscopic follow-up of 11 candidates from the MGQPC catalog confirms 6 dual quasars and 3 projected quasars, with discussion of prior survey misses and future strategies.