TNG Allocations - Period AOT42/2020B
Below are listed the time allocations for semester AOT42/2020B (October 1, 2020 -- March 31, 2021). The schedule of the semester can be found here
INAF TAC |
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Programme | PI | Title | Instrument | Allocation (hours) |
A42TAC_1 | W. Boschin | The "sausage" cluster and its close companion. A spectacular case study in the context of cluster accretion | DOLORES+MOS | 12 |
A42TAC_2 | A. Grazian | Finding the brightest Cosmic Beacons in the Equatorial Stripe | DOLORES | 9 |
A42TAC_6 | M. Lazzarin | Spectroscopic investigation of newly discovered comets as background for the ESA Comet Interceptor mission | DOLORES/NICS | 17 |
A42TAC_8 | E. Mazzotta Epifani | Unveiling the nature of (65803) Didymos, the asteroid target of the NASA/DART space mission | DOLORES | 20 |
A42TAC_12 | S. Antoniucci | GHOsT (GIARPS High-resolution Observations of T Tauris): toward a statistical analysis of the accretion rate | GIARPS/NICS | 20 |
A42TAC_13 | R. Middei | The first NIR very high spectral resolution observations of active galaxies: the study of outflows | GIANO-B/NICS | 17 |
A42TAC_14 | G. Cescutti | Measuring at Intermediate metallicity Neutron Capture Elements (MINCE) | HARPS-N | 9 |
A42TAC_15 | V. Ripepi | Spectroscopic follow-up of Gaia and OGLE newly discovered Classical Cepheids | HARPS-N | 18 |
A42TAC_17 | V. Testa | Probing the most luminous QSOs in the universe by completing the NIR photometry of the WISSH sample | NICS | 9 |
A42TAC_19 | P. D'Avanzo | Hunting for kilonovae in the local Universe with TNG | DOLORES/NICS | 10 |
A42TAC_20 | M. Rainer | A precise characterisation of the ARIEL stars II - the sequel | HARPS-N | 9 |
A42TAC_21 | L. Izzo | Are Classical Novae the progenitors of Supernovae Ia ? | DOLORES | 7 |
Nordic programmes: | ||||
A42TAC_22 | E. Knudstrup | Planetary Migration Patterns | HARPS-N | 16.25 |
A42TAC_27 | A. Bello-Arufe | What is in Hell? - Studying the atmosphere of HAT-P-70b, one of the hottest exoplanets. | HARPS-N | 5.5 |
A42TAC_28 | C. von Essen | Constraining the boundaries of the Neptune desert via accurate masses | HARPS-N | 27 |
Confirmed Large Programmes: | ||||
A37TAC_31 (GAPS) | G. Micela | GAPS2: the origin of planetary systems diversity | GIARPS | 306 |
A37TAC_13 | L. Origlia | Stellar Population Astrophysics: the detailed, age-resolved chemistry of the Milky Way disk | GIARPS | 81 |
Confirmed Long Term Programmes: | ||||
A41TAC_8 | A. Pastorello | Probing the latest stages of the evolution of massive stars through observations of interacting transients | DOLORES/NICS | 20 |
A41TAC_18 | S. Piranomonte | Follow-up of electromagnetic counterparts of gravitational wave sources at TNG | DOLORES/NICS | 30 |
A41TAC_54 | R. Silvotti | Wanted dead and alive. The first MS+WD binary with a living and a dead planetary system | HARPS-N | 3 |
Spanish CAT |
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Programme | PI | Title | Instrument | Allocation (nights) |
CAT19A_162 | G. Nowak | Follow-up of TESS small planet candidates: Precise masses as fundamental parameter for planet structure, distributions and in-depth atmospheric studies. | HARPS-N | 10 |
CAT20B_23 | L. Beitia Antero | Characterization of nearby High Radial Velocity Stars | HARPS-N | 2 |
CAT20B_41 | E. Pallé Bago | Mass determination of single-transit warm Jupiters from TESS | HARPS-N | 6 |
CAT20B_80 | N. Casasayas Barris | Characterising the day-side of brown dwarfs and ultra hot Jupiters | GIARPS | 5 |
CAT20B_90 | M. Oshagh | Distinguishing brown dwarfs and giant planets via obliquity measurements from time-resolved | HARPS-N | 0.5 |
CAT20B_112 | A. Domínguez | Spectroscopic observations of gamma-ray detected blazar candidates | DOLORES | 4.5 |
IAC SERVICE | 3 |
OPTICON |
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Programme | PI | Title | Instrument |
Allocation (nights) |
OPT20B_10 | P. Tisserand | Spectroscopic follow-up of rare dusty RCB stars candidates | DOLORES | 4 |
ITP |
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Programme | PI | Title | Instrument |
Allocation (nights) |
ITP20_3 | A. Caratti | Resolving the Inner Structure of Proto-Planetary Discs: a Combined GIARPS/TNG-GRAVITY/VLTI Survey | GIARPS | 3.5 |
ITP20_7 | R. Kotak | Exploring exotic and extreme transients with GOTO | DOLORES | 3 |