README web version of /home/usg/OPS/MTS/readme_xml/readme_83071900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Dear colleagues,
this proposal is in support of observatory program 278.D-5008. The UVES observations
will be used to derive Teff and log g for LTT 4816. In combination with spectra
obtained with SINFONI and a model of the stellar atmosphere the star will then complement
a set of 12 standard stars already established for X-shooter flux calibration from
320-2500 nm.
Finding chart: Please note the star has high proper motion of about 0.5 arcesc/year.
We have thus used a optical DSS 2 image for the finding chart since this is the
source closest in time.
We ask to execute the two OBs in sequence if possible.
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 specified the S/N ratio at given wavelength in the User Comments
field of each OB?
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 ?
If you need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:30 2009
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