README web version of /home/usg/OPS/MTS/readme_xml/readme_81027000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The main purpose of this proposal is the spectroscopic follow-up of three
planetary transiting candidates located in the field of the open cluster NGC 6253.
We want to derive RV variations to constrain the masses of the transiting objects,
and estabilish candidates' cluster membership. Moreover, we will maximize the
scientific return of our survey, targeting also a sample of variable stars detected
in our photometric database, as long as probable cluster members and field stars,
thanks to the UVES/MEDUSA configuration.
Because of the location of our transiting candidates it was necessary to prepare
two different configurations for FLAMES which have been labelled with the letters
A, and B. We prepared 4 couples of OBs of type A and B, which are exactly the same,
apart from the names used to distinguished them.
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 15:40:23 2009
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