README web version of /home/usg/OPS/MTS/readme_xml/readme_80503600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The DDT observations with FLAMES-UVES serve to perform radial velocity
measurements
of a transiting extrasolar planet candidate. The period of the object is close to
2.5 days.
The star has a magnitude of I=13.97.
Eight identical observing blocks are prepared that should be observed at least 4
hours apart.
It would be fine to observe 8 nights in a row, once a night. Or, 4 nights in a row,
twice a night (~4 hrs apart). Or a combination of the above.
Note that the PI will be out of email contact from December 23 until January 3.
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 15:40:22 2009
If you have comments, please contact usd-help@eso.org