README web version of /home/usg/OPS/MTS/readme_xml/readme_84015400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is observations of multiple detached eclipsing binaries in the two
open clusters NGC2243 and NGC2506. The aim is to measure masses of the stars from
the multi-epoch radial velocities. In addition to the binaries, free fibers are
used to determine cluster membership for single cluster stars. UVES fibers are used
for metallicity measurements.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
For each cluster there are 15 epochs of FLAMES observatons of the eclipsing
binaries. On any given night a maximum of 1 OB for each cluster should be executed.
That is one OB starting with NGC2243_epoch... and one OB starting with NGC2506_epoch...
Furthermore please make sure that all 15 OBs for one cluster are not executed within
15 days, but allow for nights with no observations, if this does not come naturally.
Optimally the time span from first to last epoch should be at least 30 days.
The 2 OBs named NGC2243_CMD1 and NGC2243_CMD2 are observations of single stars to
determine their cluster membership from radial velocities. These OBs are not time
critical and can be executed on either the same or separate nights.
Special Execution Requirements
The observations are of a mildly time critical nature, as specified in
the 'Time-Critical Aspects' section.
The finding charts for NGCXXXX_epochY OBs all show the allocated objects for epoch1,
since most objects are identical for all epochs. The VLT Guide star is indicated
with a red tilted square, the FACB stars are marked with red squares, and the field
center is marked with a wide blue circle. All these are identical for all observations
of this kind. This does not apply to the two OBs NGC2243_CMD1 and NGC2243_CMD2,
which have different pointings and FACB stars, and therefore different finding charts.
Special Calibration Information
ToO Information
ToO Activators List
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
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 15:40:31 2009
If you have comments, please contact usd-help@eso.org