README web version of /home/usg/OPS/MTS/readme_xml/readme_82036300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a simple survey project aimed at obtain detailed chemical abundances
for a sample of 26 stars belonging to the leading tail of the Sagittarius dwarf
Spheroidal galaxy tidal streams.
26 OBs were submitted, one per target. The OBs are identical each other but for
the coordinates and the exposure times. Exposure time is ~30min per target brighter
than V=16.6 and ~1hr for target fainter than that. Targets have K magnitudes in
the range 11.6-12.8. There are no measured V magnitudes for our targets. However,
we estimate the V magnitudes to be in the range V=15.6-17.1. K and estimated V magnitudes
are given in the OBs "user comments" field.
There are no particular priorities among the targets and observations are not critically
affected by the observing condition as long as the target S/N is obtained (S/N~>25@600nm).
Waiver Requests
Three waiver request were approved:
1- we asked to observe a different target list. We realized that
a few targets were to be preferred (due to their color, reddening and
magnitudes) to others and that a few targets were to be excluded due to
the presence of one or few close/bright nearby stars.
2- we asked to use the following
UVES instrument setup: DIC2 437+760 (instead of DIC-1 390+580).
Our targets have temperatures below 4000K. As such their spectra might show TiO
bands which might complicate the chemical abundance analysis. However, TiO bands
are negligible in large part of the red range in the new setup.
3- we asked to override the 1hr limit. A few of our target requires integration
times of ~1hr and,hence, ~1h10m of total execution time.
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 15:40:27 2009
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