README Template 73.1
(please do not delete the README Template Version line!)

ESO Programme ID: 073.A-9012(A)
Principal Investigator Name: Alexei Kniazev
Principal Investigator E-mail Address: kniazev@mpia.de
Principal Investigator Telephone Number: +49-6221-528-387
Principal Investigator Postal Address: Max-Planck-Institute for Astronomy /
  Koenigstuhl 17 / D-69117 Heidelberg / Germany

Instrument: WFI
OPC Priority Class: B
OPC Approved Total Execution Time: 37.0
Estimated Total Execution Time (including overheads): 30.0

README File Submission Date: 28 June 2004

Programme Description
=====================

General Overview
----------------

This is a simple imaging program of some nearest galaxies in narrow-band
filters.

We submitted 9 OBs for observations of spectrophotometric standard star
Feige110 in narrow-band filters (OBs with names Stand_1 ... Stand_9).
We request to observe one from these 9 OBs per night when observations
for our program will be done. Not all of them should be observed from this
point of view.

But we request to observe OB SagDIG_ST with this star during a night when
OB SagDIG_OIII will be observed.


Approved Waiver Request Summary
-------------------------------

None


Critical Observing Condition Constraints
----------------------------------------

None


Time Critical Aspects
---------------------

We submitted 9 OBs for observations of spectrophotometric standard star
Feige110 in narrow-band filters (OBs with names Stand_1 ... Stand_9).
We request to observe one from these 9 OBs per night when observations
for our program will be done. Not all of them should be observed from this
point of view.

But we request to observe OB SagDIG_ST with this star during a night when
OB SagDIG_OIII will be observed.



Special Calibration Information
-------------------------------

We have submitted two sets of sky and dome flatfield OBs to obtain flatfield
frames for the narrow-band filters.


ToO Information
---------------

This is not a ToO programme.


Pre-Imaging Requirements
------------------------

No pre-imaging is required for this programme.

Source of preimaging: Not applicable

OB Information
==============

List of Science OBs
-------------------
(for ISAAC imaging, please indicate the magnitude of the brightest star
in the field for each OB)

Total Number of Submitted Science OBs: 29


List of Calibration OBs with Associated Science OBs
---------------------------------------------------

Total Number of Submitted Calibration OBs: 12


OB Compliance Checks
====================

(Y = Yes, N = No, NA = Not Applicable)

Do all your OBs comply with the instrument specific requirements
listed on the instrument specific Phase 2 Web pages ? [Y]

Do all your Finding Charts comply with the both the general and
instrument-specific finding chart requirements? [Y]

If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars ? [Y]

Have you included OBs for any calibrations that you need but 
which are not a part of the Calibration Plan?  [Y]

[FORS only] Do all your FORS OBs use only the allowed detector read-out
modes listed on the FORS1/FORS2 Phase 2 Web pages? [NA]

[FORS only] Do all your FORS MOS/LSS OBs contain the mandatory
"through-slit image" template? [NA]

[UVES only] Do all your UVES OBs use only the allowed templates listed
on the UVES Phase 2 Web pages ? [NA]

[ISAAC only] Did you indicate the magnitude of the brightest star in the
field for ISAAC imaging observations? [Y]

[ISAAC only] If you submitted OBs for standard stars, did you
use the provided StandardStar templates? [Y]

[FLAMES only] Did you specify the hour angle range for which your Target
Setup files are valid ? [NA]

[VIMOS only] Did you specify suitable guide stars for all your OBs
using Guidecam? [Y/N/NA]

[VIMOS only] Did you check that the chosen guide stars are suitable for
all the offset positions and that they do not produce unacceptable
vignetting of the field of view? [NA]


If you answered "NO" to any of these questions, please revise your 
OBs *before* submission.