| Ref. CAT | IP | Awarded # nights | Instrument | Large program | Program |
|---|
| 11-INT2/22B | Pablo Rodríguez Gil | 5 B | IDS | - | Confirming the reliability of photometrically derived stellar masses in close binaries |
| 36-INT7-D/22B | Alberto Javier Castro Tirado | 30 A (1hrs) | WFC | - | GTC follow-up of gravitational radiation sources in the Multi-messenger Era |
| 130-INT10/22B | Tomás Müller Bravo | 3 B + 7 B | IDS | - | Spectroscopy for the Classification and Characterization of Infant Supernovae with INT in the optical |
| 131-INT11/22B | Javier Román García | 6 D | WFC | - | Color, morphology and star formation rate of dark-matter poor ultra-diffuse galaxies |
| 133-INT14/22B | David Jones | 2 G + 2 B | WFC | - | Recently discovered post-common-envelope binary central stars of planetary nebulae |
| 134-INT15/22B | Eduardo Martin Guerrero de Escalante | 3 G | IDS | - | Ultra metal poor M-type benchmarks |
| 135-INT16/22B | Ignacio Trujillo Cabrera | 10 D + 3 G | WFC | - | Deep u-band and Halpha imaging of the LIGHTS galaxy survey |
| 139-INT19/22B | Jorge Casares Velázquez | 5 D + 5 G + 2 B | IDS | - | Does V404 Cyg contain a massive BH? |