Target of Opportunity Proposals in Period 65
This list of OPC approved Target of Opportunity Proposals (ToOs) is updated every observing period. The ESO ToO Policy is available from a separate document.
65.H-0212 | Covino, S., Cimatti, di Serego Alighieri, Ghisellini, Haardt, Israel, G.L., Lazzati, Pasquini, Saracco, Stella, Tagliaferri, Vanzi, Vietri, Ricker: 'Variable Polarization of Gamma Ray Burst Optical Afterglows: | |
Obs. Run | Telescope / Instrument | Time Allocated |
A | UT1-ANTU / FORS1 | 12h |
65.H-0215 | Lazzati, Campana, Celotti, Chincarini, Cimatti, Covini, S., di Serego Alighieri, Ghisellini, Haardt, Israel, G.L., Pasquini, Saracco, Stella, Tagliaferri, Vanzi, Vietri:: 'Disclosing the Connection between Gamma-Ray Bursts and Supernovae'' | |
Obs. Run | Telescope / Instrument | Time Allocated |
A | UT2-KUEYEN/ FORS2 | 6h |
B | UT1-ANTU / ISAAC | 3h |
65.H-0247 | Chaty, Mirabel, Marti, Rodriguez, Ogley: 'ToO Infrared and Optical Observations of Galactic Hard X-Ray Sources' | |
Obs. Run | Telescope / Instrument | Time Allocated |
A | NTT / SOFI | 13h |
B | NTT/ EMMI | 5h |
65.H-0426 | Della Valle, Pasquini, Cappellaro, Turatto: 'Searching for Progenitors of type Ia Supernovae' | |
Obs. Run | Telescope / Instrument | Time Allocated |
A | UT2-KUEYEN/ UVES | 12h |
B | 1.5m/ FEROS | 1n |
65.H-0468 | Lundqvist, Leibundgut, Baron, Fransson, Nomoto: 'Early evolution of a bright supernova' | |
Obs. Run | Telescope / Instrument | Time Allocated |
A | UT2-KUEYEN/ UVES | 9.5h |
165.H-0464 | van den Heuvel, Frontera, Hjorth, Castro-Tirado, Greiner, Vreeswijk, Rol, Pedersen, Pian, Gorosabel, Palazzi, Masetti, Kouveliotou, Wijers, Fruchter, Wiklind, Jaunsen, Courbin, Augusteijn, Boer, Atteia, Ricker, Piro, Heise, Hurley, Danziger (Large Programme with ToO status): 'The Physics of Gamma-Ray Bursts (GRBs) and the Nature of their Hosts' | |
Obs. Run | Telescope / Instrument | Time Allocated |
A | UT1-ANTU/ FORS1 | 20h |
B | UT2-KUEYEN/ FORS2 | 5h |
C | UT1-ANTU/ ISAAC | 20h |
D | UT2-KUEYEN/ UVES | 5h |
E | NTT/ SOFI | 30h |
G | 1.5mD/ DFOSC | 0.6n |
H | 2.2m/ WFI | 6h |
I | 3.6m/ EFOSC2 | 18h |