README web version of /home/usg/OPS/MTS/readme_xml/readme_83063301
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program is designed to continue a radial velocity survey for binaries
within the young massive galactic cluster Wd1.
The initial phase of observations were obtained in 2008 and were designed to search
for short period binaries, while this extention is designed to search for systems
with orbital periods of months to years.
Consequently we request that this run 383.D-0633(A) be executed in the first half
(Aril-June) of the semester, with the second 383.D-0633(B) executed in the second
half (July-Sept), ideally with 3 or more months separating them in order to optimise
the length of the observational baseline.
This constraint reflects the `Time Intervals' selected in each of the OBs for both
runs.
However, if this is not possible due to adverse weather/instrumental problems/scheduling
constraints we request that these conditions be relaxed such that both runs are
executed. In this respect if it is not possible to execute 383.D-0633(A) in the
first half of the semester then please attempt it in the second half as well as
83.D-0633(B). Likewise, please ignore our contraint that both runs be executed 3months
appart if this would preclude both runs being executed.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
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 15:40:30 2009
If you have comments, please contact usd-help@eso.org