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- Gaia16alo is a Type II SN (2016)
- Gaia16amw is a previously missed, old core-collapse SN at 20 Mpc (2016)
- Gaia16apd-a link between fast and slowly declining type I superluminous supernovae (2017)
- Gaia17biu/SN 2017egm in NGC 3191: The Closest Hydrogen-poor Superluminous Supernova to Date Is in a "Normal," Massive, Metal-rich Spiral Galaxy (2018)
- Galaxy and Mass Assembly (GAMA): Low-redshift Quasars and Inactive Galaxies Have Similar Neighbors (2023)
- Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1 < z < 0.35 (2022)
- Galaxy group-associated distances to very high energy gamma-ray emitting BL Lacs KUV 00311−1938 and S2 0109+22 (2024)
- GALEX AND PAN-STARRS1 DISCOVERY OF SN IIP 2010aq: THE FIRST FEW DAYS AFTER SHOCK BREAKOUT IN A RED SUPERGIANT STAR (2010)
- Gamma-ray and optical oscillations of 0716+714, MRK 421, and BL Lacertae (2017)
- Gamma-ray Excess from a Stacked Sample of High- and Intermediate-frequency Peaked Blazars Observed with the MAGIC Telescope (2011)
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