WFI

Last update of this page: Mon Apr 2 13:44:56 2007

PHOT	CLR	THN	THK	Seeing & Airmass Constraints:
29 OB(s)	68 OB(s)	--	--	Seeing < 1.50 Airmass < 1.50

Last update of the USG file: Oct 12 15:00:08 2005
Major Instrument Modes: WFI with BVR filters

RA Range: 0.5h - 7.4h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
1.2 2CLR 1.5 0.4 120

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

 
 

===> Latest news (October 2005): The user has accepted a relaxation of 
constraints to 1"5 seeing so that the runs gets some chance of advancing.

21.12.2004: PI stressed out on the quite importance of observations
	    of fields 5 and 6 (BVR filters) because the bulk
	    of their complementary observations are available
	    only in these fields.

This is the second run of an imaging Large Program on the ELAIS S1 field.
The program  planned to observe four different subfields (called from
Field 5 to Field 16) in three bands B, V, R.

Period71:
This is the third run of an imaging Large Program on the ELAIS S1 field.
The program planned to observe 6 different subfields (called Field 17, 18,
19, 20, 21, 22) in three bands B, V, R.

The astrometric calibrator Field D must be executed before November.
If the observations will be allocated in November or later PI requests to
execute Field E. In total prgram need only ONE single astrometric
field to be observed.

PCa requested in B,V and R filters.

The program has Time Critical Aspects and requested for additional
photometrical calibrations and OBs for it. See for details README file.
 
 

Run status page 168.A-0322A

Approved README of this run: