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Time Critical |
Last update of this page: Tue Oct 7 13:41:37 2008
Run State: TERMINATED/EP
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? | |
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Special Remarks:
The spectroscopy (with FORS2, Run A, scheduled in class B) will trigger the photometry (with FORS1, Run B, class A) as a "time critical" observation for execution "as soon as possible" - ideally during that night.
Abstract for MTS:
FORS2 LSS of SNe in their nebular phase. PI has added additional OBs for photometry on FORS2.
Please take into account user priorities for the execution of the spectroscopic OBs:
Target Priority
-------------------
SN2006aj 1
SN2005hk 2
SN2006F 3
SN2006T 4
-------------------
For the same object, there are a sequence of obs to be observed in the preferred time intervals which are specified in the
following table.
Dates | FORS2 spec OB | Corresponding FORS1 ima OB | Alternative FORS2 ima OB
SN2006aj
--------
21-30 Nov 06 | spec_F2_300V_06aj_p1 | phot_F1_VR_06aj | phot_F2_VR_06aj
21-30 Nov 06 | spec_F2_300V_06aj_p2 | |
21-30 Nov 06 | spec_F2_300I_06aj_p1 | |
21-30 Nov 06 | spec_F2_300I_06aj_p2 | |
01-31 Dec 06 | spec_F2_300V+gg375_06aj_p1 | phot_F1_V_06aj_p1 | phot_F2_V_06aj_p1
01-31 Dec 06 | spec_F2_300V+gg375_06aj_p2 | |
01-31 Dec 06 | spec_F2_300V+gg375_06aj_p3 | |
01-15 Feb 07 | spec_F2_300V+gg375_06aj_p4 | phot_F1_V_06aj_p2 | phot_F2_V_06aj_p2
01-15 Feb 07 | spec_F2_300V+gg375_06aj_p5 | |
01-15 Feb 07 | spec_F2_300V+gg375_06aj_p6 | |
01-15 Feb 07 | spec_F2_300V+gg375_06aj_p7 | |
SN2005hk
--------
21-30 Nov 06 | spec_F2_300V+gg375_05hk_p2 | |
01-31 Dec 06 | spec_F2_300V+gg375_05hk_p3 | phot_F1_VR_05hk_p3 | phot_F2_VR_05hk_p3
01-31 Dec 06 | spec_F2_300V+gg375_05hk_p4 | |
01-31 Dec 06 | spec_F2_300V+gg375_05hk_p5 |
SN2006T
-------
01-28 Feb 07 | spec_F2_300V+gg375_06T | phot_F1_V_06T-0 | phot_F2_V_06T
Important Note: please, follow the object priorities given by the PI in the OBs:
078.D-0246B.03.WAV: Waiver was approved on 17.08.06
We kindly require that the photometry could be alternatively executed with FORS2 for some or all targets.
JUSTIFICATION: Although we indicated in the Phase I Proposal that we want photometry with FORS1, we also indicated (Box 3 of Phase 1 proposal) the
possibility of interchanging the instruments, should this be more convenient for the simultaneous scheduling of spectroscopy (Run A) and
photometry (Run B). Therefore - although our primary request is for photometry with FORS1 - we request that photometry is performed with FORS2
for those targets and/or epochs for which ESO sees it easier to schedule both spectroscopy and photometry with the same instrument (FORS2).
For target SN2006jc : this is faint, so LSS is done with blind offset from star number 1, as detailed in the finding chart.
The user kindly asks to use the OB "CAL_GD71_MARCH_I" for the spectrophotometric calibration during
the same night of the OB "SN2006jc_MARCH_I_1", because he reports some problem with previous spectrophotometric
standard calibrations in the red part of the spectrum.
README of this run:
Web version of approved README readme_78024600.html