README web version of /home/usg/OPS/MTS/readme_xml/readme_81081700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Five cold (Teff~5000) metal poor subdwarf stars are observed at high S/N,
high resolution to measure Mg isotopic split in the MgH band near 513 nm. Typical
requrement for final S/N (on coadded spectra) varies between 150 and 350 depending
on the star characteristics.
All the stars are nearby halo dwarfs, thus show high proper motions. Since finding
charts (from DSS2 plates) can be more than 15 years old, many stars may have significantly
moved with respect to nearby sources. Coordinates at 2000 equinox and epoch are
provided as well as proper motions, extracted from Simbad. Proper motions appear
to be accurate, comparing DSS1 position against 2MASS.
This program is a re-edition of 079.D-0734 which went almost unexecuted due to bad
weather conditions.
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 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 15:40:25 2009
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