README web version of /home/usg/OPS/MTS/readme_xml/readme_78032300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The observing program consists of high-resolution observations of a sample
of 115 RGB stars in 2 fields in the LMC (a field in the "LMC Outer" disk, and a
field centered on the "LMC bar"):
* 5 repeated OBs to observe the LMC_Outer field with GIRAFFE H14A setup + UVES_580.
THIS IS OUR FIRST PRIORITY
* 5 repeated OBs to observe the LMC_Bar field with GIRAFFE H11 setup + UVES_580
(uv1: 7 uves targets)
* 5 repeated OBs to observe the LMC_Bar field with GIRAFFE H11 setup + UVES_580
(uv2: 7 different uves targets)
* 10 repeated OBs to observe the LMC_Outer field with GIRAFFE H11 setup + UVES_580.
Each of these 4 subsets of OBs will produce observations that we will CO-ADD to
obtain our final data. We therefore prefer that each subset is COMPLETED before
the next is started (rather than getting all setups covered with lower S/N).
Both fields have already been sucessfully observed (P72 and P74 respectivelly) with
the same guide-star and fiducial stars.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
Did you specify in your OBs the hour angle range for which your Target
Setup files are valid ?
Did you specify in your OBs the magnitudes of FACBs and Guide Star for
all your fields ?
Are the FACBs and Guide Star in the brightness ranges specified in the
FLAMES manual ?
Did you enter the expected signal to noise in your OBs ?
Last creation of page: Tue Oct 6 15:40:15 2009
If you have comments, please contact usd-help@eso.org