README web version of /home/usg/OPS/MTS/readme_xml/readme_81062000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We are completing our program 079.B-0672(A) by obtaining
UVES spectra for the remaining four of six very metal-poor stars in
the nearby dwarf spheroidal galaxies Sculptor, Fornax and Sextans
These stars have been identified as the most metal-poor stars in our
DART Calcium triplet survey of about 2000 stars, which offers the most
complete metallicity distribution to date. We will derive accurate
abundances for a wealth of elements, thereby constraining the earliest
phase of star formation in these galaxies and enabling a careful
comparison to the metal-poor stars in the Milky-Way.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
The only particularity of these observation concerns
the guide camera that we set in RED while we are observin with DIC#1 3900-580.
Indeed the red part of the stellar spectra constitute our primary target. In order
to limit the effect of the atmospheric diffraction, we open the blue slit to 1.2
arcsec (red slit is 1arcsecc wide) and we require observations at airmasses below
1.6.
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 15:40:24 2009
If you have comments, please contact usd-help@eso.org