| Ref. CAT | PI | Awarded number of nights | Instrument | Large program | Title |
|---|
| 4-INT1-A/20B | Ovidiu Vaduvescu | 5 A (1hrs) | WFC | - | Targeting the low-end of the NEA brightness distribution: the INT 1000 square degrees survey |
| 4-INT2-B/20B | Ovidiu Vaduvescu | 3 A + 2 A | WFC | - | Targeting the low-end of the NEA brightness distribution: the INT 1000 square degrees survey |
| 47-INT3/20B | Jairo Mendez Abreu | 5 G | WFC | - | THE LOW-SURFACE BRIGHTNESS STRUCTURE of BULGELESS GALAXIES |
| 81-INT4/20B | Matteo Monelli | 5 G | WFC | - | Homogeneous photometry in the Gaia era: poorly studied stellar clusters |
| 102-INT6-A/20B | Paula Izquierdo Sánchez | 3 D + 1 G | IDS | - | A critical test of compact binary evolution theory with a volume-limited white dwarf binary sample |
| 102-INT7-B/20B | Paula Izquierdo Sánchez | 3 G | IDS | - | A critical test of compact binary evolution theory with a volume-limited white dwarf binary sample |
| 134-INT8/20B | Ignacio Trujillo Cabrera | 6. D + 9. D | WFC | - | Is there a missing stellar halo problem? |
| 136-INT9-A/20B | Ovidiu Vaduvescu | 10. A (1.hrs) | WFC | - | Targeting the low-end of the NEA brightness distribution (special call 2020B) |
| 140-INT12/20B | Alvaro Alvarez Candal | 6. A (4.5 hrs) + 6. A (4.5 hrs) | WFC | - | Studying surface properties of Trojans |
| 141-INT13/20B | Nicolas Lodieu | 5. A | WFC | - | Formation origins of brown dwarfs from rotation rates |
| 143-INT14/20B | Ignacio Negueruela Díez | 3. A | IDS | - | New distant young open clusters in the UBC database |