TNG Allocations - Period AOT30/2014B
Below are listed the time allocations for semester 2014B/AOT30 (September 1, 2014 - February 28, 2015). See the schedule of the period.
INAF TAC
Programme | PI | Title | Instrument | Allocation (hours) |
A30TAC_8 | S. Antoniucci | EXORCISM - Observations of EXor young variables in outburst | DOLORES/NICS | 5 |
A30TAC_9 | S. Faggi | Search for organic ices in the coma of the new Oort comet C/2013 X1 (PANSTARRS) | DOLORES/NICS | 8 |
A30TAC_13 | S. Albrecht | Detecting transiting close-in Super-Earth planets from the K2 mission | HARPS-N | 16 |
A30TAC_14 | T. Pursimo | Spectroscopy and Flux Evolution of Rapid Gamma-ray Flaring Sources | DOLORES | 20 |
A30TAC_16 | V. D'Elia | Exploring the Universe with Gamma-Ray Burst Afterglows | DOLORES/NICS | 18 |
A30TAC_18 | E. Kankare | Studies of peculiar supernovae with NOT and TNG - near-IR monitoring | NICS | 12 |
A30TAC_19 | E. Palazzi | Spectroscopic and imaging follow-up of gravitational radiation sources with TNG | DOLORES/NICS | 12 |
A30TAC_22 | G. Cupani | Reference QSO spectra for precision cosmology: accurate flux calibration of echelle observations | DOLORES | 10 |
A30TAC_25 | G. Terreran | Studies of peculiar supernovae with TNG and NOT - optical monitoring | DOLORES | 28 |
A30TAC_26 | G. Bonnoli | Polarimetric monitoring of MAGIC blazars | DOLORES | 12 |
A30TAC_27 | D. Malesani | Fast radio bursts: Our first chance to discover their optical counterparts | DOLORES/NICS | 14 |
A30TAC_29 | J. Telting | Planetary companions to sdB stars | HARPS-N | 10 |
Spanish CAT
Programme | PI | Title | Instrument | Allocation (nights) |
CAT14B_7 | T. Shahbaz | Polarimetry as a tool for measuring black hole masses in low-mass X-ray binaries | DOLORES (PAOLO) | 1 |
CAT14B_27 | G. Bernabeu Pastor | Unveiling the infrared donors in obscured high mass X-ray binary candidates | NICS | 1 |
CAT14B_69 | I. Ribas Canudas | High-precision radial velocity survey to detect low-mass planets around M-type stars | HARPS-N | 7 |
CAT14A_83 | R. Rebolo López | Searching for Earth-mass planets in solar-type stars with both HARPS-N | HARPS-N | 6 |
CAT14B_94 | R. Alonso Sobrino | The shortest and the longest period planets in the CoRoT-24 system | HARPS-N | 1.5 |
CAT14B_95 | D. Tescaro | Constraining the Extragalactic Background Light through gamma-ray BL Lacs objects | DOLORES | 4 hr |
CAT14B_100 | D. Tescaro | Revealing the nature of unidentified gamma-ray sources | DOLORES | 2 |
CAT14B_109 | H. J. Deeg | Can atmospheric evaporation explain the diversity of low-mass planets? | HARPS-N | 2 |
CAT14B_121 | E. Pallé Bago | Characterization of Transiting Exoplanetary Systems Unveiled by K2 | HARPS-N | 2 |
CAT14B_153 | J. Gorosabel Urkia | Detecting the most distant objects of the Universe with the TNG | DOLORES/NICS | 4 hr |
CAT14B_162 | Z. Modroño Berdiñas | Cool tiny beats IV: Small planets, activity and pulsation in M dwarfs | HARPS-N | 3.5 |
CAT13B_145 | E. Villaver | TAPAS: Tracking Advanced PlAnetary Systems with HARPS-N | HARPS-N | 5 |
OPTICON
Programme | PI | Title | Instrument | Allocation (nights) |
OPT14B_7 | C. Inserra | “Super-bright” optical transients: giant supernovae in dwarf galaxies | DOLORES | 1 |
OPT14B_33 | A. Santerne | The density diversity of planets around small stars | HARPS-N | 4 |
OPT14B_45 | M. Konacki | The radial velocity survey for circumbinary extrasolar planets | HARPS-N | 6 |
OPT14B_66 | D. Anderson | Testing spin-orbit alignment in the weak tidal regime | HARPS-N | 1 |
CCI ITP
Programme | PI | Title | Instrument | Allocation (nights) |
ITP14_3 | J.I. González Hernández | Towards the detection of super-Earth and Earth like planets around M-dwarf stars | HARPS-N | 4 |
ITP13_8 | J.A. Rubiño Martín | The Planck SZ Galaxy clusters: building a reference sample for Cosmology | DOLORES+MOS | 3 |