Ref. CAT | PI | Awarded number of nights | Instrument | Large program | Title |
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6-INT3/21A | Cristina Ramos Almeida | 4 D | WFC | - | Why do AGN discs have larger rotation support than non-active twin galaxies? |
7-INT4-A/21A | Jesús Maíz Apellániz | 1 A | IDS | - | The optical extinction law with IDS/INT spectrophotometry |
7-INT5-B/21A | Jesús Maíz Apellániz | 2 A | IDS | - | The optical extinction law with IDS/INT spectrophotometry |
7-INT6-C/21A | Jesús Maíz Apellániz | 2 A | IDS | - | The optical extinction law with IDS/INT spectrophotometry |
7-INT7-D/21A | Jesús Maíz Apellániz | 1 A | IDS | - | The optical extinction law with IDS/INT spectrophotometry |
21-INT10/21A | Laura Scholz Díaz | 4 D + 7 G | IDS | - | Do black holes regulate the baryonic cycle of dark matter halos? UV-powered star formation histories of golden mass galaxies |
36-INT11/21A | Matteo Monelli | 3 A + 3 A | WFC | - | Homogeneous photometry in the Gaia era: poorly studied stellar clusters |
54-INT13/21A | Ovidiu Vaduvescu | 4 A | IDS | - | Near Earth asteroids in cometary orbits |
63-INT14/21A | Pablo Rodríguez Gil | 3 D + 4 G | IDS | - | A critical test of compact binary evolution theory with a volume-limited white dwarf binary sample |
81-INT16/21A | Alejandro Lumbreras Calle | 1 D | IDS | - | Uncovering local extreme emission line galaxies with J-PLUS: analogues of very high-redshift systems |
92-INT18/21A | Isabel Perez Martin | 4 D + 3 D | WFC | - | The environment of Void Galaxies |
96-INT19/21A | David Jones | 5 G | WFC | - | Exploiting Gaia to build a statistically-significant sample of close-binary central stars of planetary nebulae |