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.


Programme PI Title Instrument Allocation
A30TAC_8 S. Antoniucci EXORCISM - Observations of EXor young variables in outburstDOLORES/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 missionHARPS-N 16
A30TAC_14 T. Pursimo Spectroscopy and Flux Evolution of Rapid Gamma-ray Flaring SourcesDOLORES 20
A30TAC_16 V. D'Elia Exploring the Universe with Gamma-Ray Burst AfterglowsDOLORES/NICS 18
A30TAC_18 E. Kankare Studies of peculiar supernovae with NOT and TNG - near-IR monitoringNICS 12
A30TAC_19 E. Palazzi Spectroscopic and imaging follow-up of gravitational radiation sources with TNGDOLORES/NICS 12
A30TAC_22 G. Cupani Reference QSO spectra for precision cosmology: accurate flux calibration of echelle observationsDOLORES 10
A30TAC_25 G. Terreran Studies of peculiar supernovae with TNG and NOT - optical monitoringDOLORES 28
A30TAC_26 G. Bonnoli Polarimetric monitoring of MAGIC blazarsDOLORES 12
A30TAC_27 D. Malesani Fast radio bursts: Our first chance to discover their optical counterpartsDOLORES/NICS 14
A30TAC_29 J. Telting Planetary companions to sdB starsHARPS-N 10



Spanish CAT

Programme PI Title Instrument Allocation
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




Programme PI Title Instrument Allocation
OPT14B_7C. Inserra“Super-bright” optical transients: giant supernovae in dwarf galaxiesDOLORES1
OPT14B_33A. SanterneThe density diversity of planets around small starsHARPS-N4
OPT14B_45M. KonackiThe radial velocity survey for circumbinary extrasolar planetsHARPS-N6
OPT14B_66D. AndersonTesting spin-orbit alignment in the weak tidal regimeHARPS-N1




Programme PI Title Instrument Allocation
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