Tiempo asignado por el CAT

Semestre 2018A

Isaac Newton Telescope

Ref. CATIPNoches ConcedidasInstrumentoLarga DuraciónPrograma
4-INT1/18ADavid Barrado Navascués4. A WFC - Dynamical Analysis of Nearby Clusters
14-INT2/18AMatteo Monelli3. D + 5. G WFC - Variable stars in the Local Group as tracers of galaxy evolution
25-INT3/18AJose Alfonso Lopez Aguerri3. D + 4. D WFC - Deep imaging on the WEAVE clusters
29-INT4-A/18AOvidiu Vaduvescu5. D WFC - Testing the EURONEAR Automated Moving Source Detection Pipeline
29-INT5-B/18AOvidiu Vaduvescu5. D (2.hrs) WFC - Testing the EURONEAR Automated Moving Source Detection Pipeline
60-INT6/18AHugo Martín Tabernero Guzmán3. G + 1. A IDS - The onset of hot bottom burning in very massive red giants
70-INT7/18ARoi Alonso Sobrino3. G + 2. A + 3. A IDS - Selecting the best hot Jupiter atmospheres with INT
75-INT8-A/18ACarlos Allende Prieto4. D 2018A + 4. G 2018AIDSonly 2018AEarly Steps of the Milky Way: Old Stars as Tracers of the Formation and Evolution of the Galactic Halo.
85-INT10-A/18AOvidiu Vaduvescu8. A + 2. A WFC - Continuing the EURONEAR Lightcurve Survey of Near Earth Asteroids