Ref. CAT |
PI |
Program |
Telescope Instrument |
Status |
19A |
19B |
20A |
20B |
---|---|---|---|---|---|---|---|---|
132-MULTIPLE-2/19A |
Paul G. Beck |
Understanding stellar Lithium abundance through ground-based high-resolution spectroscopy (Hermes/Mercator) and space Asteroseismology (Kepler) |
MERCATOR/HERMES |
LP |
12 n A |
- |
12 n A |
- |
141-MULTIPLE-2/19A |
Francisco Javier Castander Serentill |
PAUS: a unique narrow band survey for cosmology and galaxy evolution |
WHT/PAUCam |
LP** |
12 n D |
12 n D** |
- |
- |
162-MULTIPLE-8/19A |
Grzegorz Nowak |
Follow-up of TESS small planet candidates: Precise masses as fundamental parameter for planet structure, distributions and in-depth atmospheric studies |
NOT/FIES |
LP |
5 n G |
10 n G |
10 n G |
10 n G |
162-MULTIPLE-8/19A |
Grzegorz Nowak |
Follow-up of TESS small planet candidates: Precise masses as fundamental parameter for planet structure, distributions and in-depth atmospheric studies |
TNG/HARPS |
LP |
5 n G |
10 n G |
10 n G |
10 n G |
** PI should read the proposal's feedback carefully.