71.D-3009(D)

PI:Della Valle/ Gilmozzi/ Madau/ Maiolino/ Mannucci/ Mason/ Panagia

71D3009D.html


Last update of this page: Mon Jun 2 17:45:06 2003
Last update of the USG file: Apr 24 10:53:42 2003


Major Instrument Modes: VIMOS IMG (pre-imaging)

RA Range: 14:21

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 0.9 2CLR 1.4 0.1 60.


Pre-imaging run? Yes! Chilean run? No! Special calibrations? No!
Time critical? Yes! ToO? No! Carry-over run? No!


Special Remarks:
It has to be executed around 04.05.03 (30+-3 days after run B).


 

Deep imaging in V and I. This run should be executed around 04.05.03,
i.e. 30+-3 days after run (B), to allow the discovery of high-z
supernovae. Given that the intervention is planned to start on 05.05,
the sooner the better.

MOS masks will be prepared as run (E).

The total execution time of the 4 OBs is 5h22m, to be completed
in two consecutive nights. Acquisition can be skipped if two OBs
are executed in a row.
 
Waivers: OBs longer that 1h (degradation allowed after 1h).

The programme is completed by run A and B (imaging to be executed
30+-3 days from each other and the present run) and C, E (follow-up
MOS).


 


Information about the progress of this run:

Run status page 71.D-3009D

README of this run:

71.D-3009D.README