CAT Ref. | PI | Awarded nights | Instrument | Large program | Programa |
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155-WHT1/19B | Jesús Maíz Apellániz | 4 A | ISIS | - | Lucky Spectroscopy: a novel technique to study close binary systems |
157-WHT3/19B | Joan Font Serra | 2 G + 1 A | GHAFAS | - | When ALMA meets GHaFaS: Confronting the resonant structure of the molecular and the ionized gas tracers in nearby galaxies. |
158-WHT4/19B | Manuel Ángel Pérez Torres | 1.5 A | LIRIS | - | Testing X-ray models for Intermediate Polars - a dynamical study of XY Ari |
164-WHT7/19B | Carlos Cifuentes San Román | 4 A (4.5hrs) | ISIS | - | Spectroscopy of poorly investigated late-type young stars in the sigma Orionis cluster |
165-WHT8/19B | Tariq Shahbaz | 1 A (4.5hrs) | LIRIS | - | Testing the jet/outflow model in a transitional millisecond pulsar |
166-WHT9-A/19B | Paula Izquierdo Sánchez | 1 D | ISIS | - | Neighbourhood watch: leave no white dwarf behind |
166-WHT10-B/19B | Paula Izquierdo Sánchez | 2 G | ISIS | - | Neighbourhood watch: leave no white dwarf behind |
167-WHT11/19B | Jonay I. González Hernández | 2 D + 2 G | ISIS | - | Early Steps of the Milky Way: Old Stars as Tracers of the Formation and Evolution of the Galactic Halo. |
168-WHT12/19B | Francisco Javier Castander Serentill | 3.5 D + 2 D | PAUCam | - | PAUS: a unique narrow band survey for cosmology and galaxy evolution |
169-WHT13/19B | Ignacio Mendigutía | 2 G | ISIS | - | The BORN survey of forming planets in disks around young stars: bright winter candidates with ISIS/WHT |
170-WHT14/19B | Jose Antonio Acosta Pulido | 5 D (4.5hrs) | ISIS | - | TRUE2: a survey of true Seyfert 2 candidates in poalrized light. Establishing a limit on the detection of hidden broad line regions. |
171-WHT15/19B | Ovidiu Vaduvescu | 2 A | LIRIS | - | Physical properties of dwarf elliptical galaxies based on deep Ks imaging |
173-WHT17/19B | Manuel Ángel Pérez Torres | 2 G | ISIS | - | A dynamical study of the black hole candidate MAXI J1820+070 |
174-WHT18/19B | Stefan Geier | 3 D (4.5hrs) | ISIS | - | Resolving the quasar selection bias with Gaia |