| Ref. CAT | PI | Allocated nights | Instrument | Large program | Title |
|---|
| 34-INT1/21B | Isabel Perez Martin | 7 D | WFC | - | The environment of Void Galaxies |
| 38-INT2/21B | Iker Gonzalez Santamaria | 4 A | IDS | - | Chemical abundances and evolutionary state of planetary nebulae with accurate distances in Gaia EDR3 |
| 44-INT3/21B | David Jones | 4 G | WFC | - | Exploiting Gaia to build a statistically-significant sample of close-binary central stars of planetary nebulae |
| 50-INT4/21B | Joao Calhau | 3 D + 3 D | WFC | - | TIHMPSS: The INT Halo Metal Poor Star Survey |
| 62-INT5/21B | Eri Tatsumi | 3 A + 3 A | IDS | - | Exploring NUV-VIS region as diagnostic of composition in primitive asteroids |
| 63-INT6/21B | Ovidiu Vaduvescu | 3 G | IDS | - | Near Earth asteroids in cometary orbits |
| 64-INT8-B/21B | Ovidiu Vaduvescu | 4 A | WFC | - | Targeting the low-end of the NEA brightness distribution: the INT 1000 square degrees survey |
| 67-INT9/21B | Ignacio Negueruela Díez | 5 A | IDS | - | Tracers of spiral structure beyond the Perseus Arm |
| 75-INT10/21B | Matteo Monelli | 3 D + 2 G | WFC | - | Homogeneous photometry in the Gaia era: undestanding the origin of globular clusters |
| 83-INT12/21B | Cristina Ramos Almeida | 4 D | WFC | - | Why do AGN discs have larger rotation support than non-active twin galaxies? |
| 94-INT13/21B | Alejandro Lumbreras Calle | 4 G | IDS | - | Uncovering local extreme emission line galaxies with J-PLUS: analogues of very high-redshift systems |