First Column: S(tatus)
  • C = 'completed'
  • P = 'partially executed'

LBC

S Object Filter Requested time Obs. time in specs Total Obs. time UT dates Notes
PI: Giallongo Proposal: Completing the first ultradeep and wide survey at z = 3
C Q0933 g 12000 12000 25600 2010-01-17;2010-02-13  
P Q0933 r 6000 1800 5400 2010-04-11  
C Cosmos g 10000 10000 10800 2010-01-17;2010-02-13,14  
C Q1623 Uspec 7200 7200 16200 2010-02-13,14;2010-06-12,14,16,17  
C Q1623 z 7200 7200 16200 2010-02-13,14;2010-06-12,14,16,17  
PI: Fiore Proposal: Large Scale Structures at high redshift in the COSMOS field
C Cosmos-P1 Uspec 10800 10800 10800 2010-02-14,15  
C Cosmos-P2 Uspec 10800 10800 10800 2010-02-15,17  
P Cosmos-P3 Uspec 10800 3600 3600 2010-02-17  
C Cosmos-P1 g 3600 3600 3600 2010-02-17  
P Cosmos-P1 r 4800 3600 3600 2010-02-17  
PI: Ferraro Proposal: Determining the binary content of Galactic globular clusters
C NGC5466 r 9000 9000 12800 2010-04-11;2010-05-07;2010-06-12,16  
C NGC5466 B 9000 9000 12800 2010-04-11;2010-05-07;2010-06-12,16  
P NGC5053 r 9000 5000 6600 2010-05-07;2010-06-12  
P NGC5053 B 9000 5000 6600 2010-05-07;2010-06-12  
PI: Rigliaco Proposal: The role of transitional and anemic disks in disk evolution: viscosity or planet formation?
C NGC2264-1 U 1800 1800 1800 2010-02-13  
C NGC2264-1 B 1800 1800 1800 2010-02-13  
C NGC2264-1 V 1800 1800 1800 2010-02-14  
C NGC2264-1 r 1800 1800 1800 2010-02-14  
C NGC2264-2 U 1800 1800 1800 2010-02-15  
C NGC2264-2 B 1800 1800 1800 2010-02-15  
C NGC2264-2 V 1800 1800 1800 2010-02-15  
C NGC2264-2 r 1800 1800 1800 2010-02-15  
C Serpens-1 Uspec 4800 4800 7200 2020-06-12,14,15,16,17  
C Serpens-1 B 2400 2400 3600 2020-06-12,14,15,16,17  
C Serpens-1 V 2400 2400 3600 2020-06-12,14,15,16,17  
C Serpens-1 R 2400 2400 3200 2020-06-12,14,15,16,17  
C Serpens-1 I 2400 2400 4800 2020-06-12,14,15,16,17  
PI: Mereghetti Proposal: Optical identification of a new class of peculiar radio transients
P LDRT Uspec 14400 9000 12600 2010-02-13,14,15,17,18  
P LDRT i 14400 1800 1800 2010-02-18  
PI: Piotto Proposal: The faintest stars in NGC 2682 (M67)
  M67 B 7200 0 10800 2010-02-18  
  M67 i 7200 0 10800 2010-02-18  
P NGC 6791 V 25200 4680 7800 2010-06-13,15,16
P NGC 6791 i 25200 4680 7800 2010-06-13,15,16
PI: Radovich Proposal: triaxial mass distribution by gravitational lensing
P A2219 B 3600 3600 3600 2010-05-07  
P A2219 V 3600 1800 3600 2010-05-07  
P A2219 r 3600 3600 3600 2010-05-07  
P A2219 i 3600 1800 3600 2010-05-07  
PI: Palazzi Proposal: Probing galaxy evolution with gamma-ray burst host galaxy
C GRB070714 U 3600 4500 4500 2010-01-17,18  
C GRB070714 B 1800 1800 1800 2010-01-17  
C GRB070714 V 1800 1800 1800 2010-01-17  
P GRB070724 B 1200 1200 1800 2010-01-18  
C GRB070724 V 1200 1200 1800 2010-01-18  
P GRB051222 U 3600 1800 1800 2010-01-18  
C GRB051222 B 1800 1800 1800 2010-01-18  

LUCIFER

S Object Filter/grat Req. time Obs. time in specs exec. time UT date Notes
PI: Mannucci Proposal: Metallicity and SFR in a unbiased sample of Lyman-Break Galaxies at z > 3
C Q1422+22 J 7200 7200 7200 2010-02-16,2010-06-13  
C Q1422+22 K 7200 7200 8100 2010-02-16,2010-06-13 serves also as preimaging for MOS mask prep
C Q1422+22 210zJHK - K 14400 14400 14400 2010-04-09,10 no Telluric for the last hour of observations
C Q1422+22 210zJHK - H 14400 14400 14400 2010-04-10,12;2010-06-13  
C HDF-N Ks   900 900 2010-02-16 preimaging for MOS mask prep, 1 field
P HDF-N 210zJHK - K 14400 12900 14400 2010-04-12;2010-05-07,2010-06-15,17  
C HDF-N 210zJHK - H 14400 14400 21600 2010-04-14;2010-06-14,17  
PI: Grazian Proposal: The Nature of MIPS 24um selected sources at z~2 in the GOODS-North field
C GOODS-N Ks   3600 3600 2010-02-16 preimaging for MOS mask prep, 4 fields
C GOODS-N1 200HK 18000 18000 18000 2010-04-09,10  
P GOODS-N2 200HK 18000 5400 10800 2010-06-16  
PI: Zamorani Proposal: Proto-clusters and obscured star formation in the most massive galaxies at z ~ 2 in the COSMOS field
C Cosmos Ks   2700 2700 2010-02-16 preimaging for MOS mask prep, 3 fields
PI: Longhetti Proposal: Were early-type galaxies denser in the past?
C S2F1-145 150_K 10800 10800 13100 2010-01-16,2010-02-17  
PI: Turatto Proposal: The chemical enrichment contribution of Supernovae from NIR/Lucifer1 nebular spectra
C SN2009hv H 7200 4800 4800 2010-01-15  
C SN2009kn 200HK 7200 1500 9000 2010-01-16  
P SN2009dc H 7200 1800 1800 2010-01-15  

-- FilippoMannucci - 18 Jan 2010

-- revised by VincenzoTesta - 22 Apr 2010
Topic revision: r11 - 22 Jun 2010, VincenzoTest
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