README web version of /home/usg/OPS/MTS/readme_xml/readme_79017800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Simple program for multi-object spectrosopy of open cluster stars. UVES
fibers point to slow rotating A and B-type stars, while the other MEDUSA fibers
point to other cluster members and observe with two HR and one LR grism. Although
centreal wavelenght for the 2 and the third setting will not be match what is set
for fiber positionning, flux losses should be still not drammatic. Note that low
resolution setting is used to see the shape of the Balmer lines, and that with this
grism, no high SNR is required.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
It would be desirable, but not critical, that the following pairs of OBs
are exectued during different night (> 1 week, if possible):
"NGC 6193 1" and "NGC 6193 2"
"NGC 6383 P2 1" and "NGC 6383 P2 2"
"NGC 6250 1" and "NGC 6250 2"
"NGC 3114 P2 1" and "NGC 3114 P2 2"
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 15:40:18 2009
If you have comments, please contact usd-help@eso.org