README Template 69.1

ESO Programme ID:			 69.D-0390(D)
Principal Investigator Name:		 Thomas Szeifert
Principal Investigator E-mail Address:	 tszeifer@eso.org
Principal Investigator Telephone Number: ++56 2 4633057 or ++56 55 435342 
Instrument:				 UVES
OPC Priority Class:			 B
OPC Approved Total Execution Time:	 2.5h
Estimated Total Execution Time (including overheads): 2.5h

README File Submission Date: 		 2002-02-01

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

General Overview
----------------
long-term time series of the Luminous Blue Variable R71 (LMC) over 9 months.
The time series should start as soon as possible - it's visible in the morning 
twilight already in July! The OBs consist of a short exposure to get H_Alpha
without saturation. The longer exposure might saturate and it's almost 
impossible to predict the line strengths in the emission lines. Since I have
the short one: Go ahead!

Waiver Request Summary
----------------------
no waivers

Critical Observing Condition Constraints
----------------------------------------
no constraints, twilight is no problem

Time Critical Aspects
---------------------
time-series must start in August latest and the frequency should be about 
WEEKLY until the end of the observation period - to be continued in P70,...

	=> COVER ALL THE PERIOD FROM July/August TO END OF SEPTEMBER ! <=

optimum frequency 7-8 days, 5-12 days gaps are fine,... but try NOT to finish
all OBs before September,...

Special Calibration Information
-------------------------------
calibration plan

ToO Information
---------------
NA

Pre-Imaging Information
-----------------------
NA

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

List of Science OBs with Associated Finding Charts
--------------------------------------------------

Total Number of Submitted Science OBs:		 9
Total Number of Submitted Finding Charts:	 1

69.D-0390D.001.ps - same target/charts for all OBs

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

Total Number of Submitted Calibration OBs:	NA

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/N/NA]? Y

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

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

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

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

[ISAAC only] Are ALL the objects in your field-of-view fainter than the 
magnitude limits specified on the ISAAC Phase 2 Web page [Y/N/NA]? NA

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

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


Destination Address for Data Products
=====================================

via Diplo-Bag to Thomas Szeifert, ESO Santiago, Alonso de Cordova 3107, CHILE