RA Range: 00:22

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.0 3THN 2.0 0.1 30

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

 
  
 
This is a MOS programme on the William Herschel Deep field, with
6 different MOS setups. The users want to establish the Tully-Fisher
relation of field spirals galaxies at intermediate red-shift, to study
their luminosity and mass evolution. The immediate objective is to
obtain the rotation curves of the target galaxies.
 
For each MOS setup, three identical exposures of 2800sec are obtained.
Each OB executes one exposure only.
Note that the users have been authorized to observe the radial velocity
standard star HD186478 within their allocated time. This should be considered
as a special calibration. 

Note that the users have supplied day-time calibration OBs. They are just
WAVECAL, and therefore can be either executed or substituted by the
automatically created calibration OBs.


 

Run status page 69.B-0278B

README of this run:

69.B-0278B.README