README web version of /home/usg/OPS/MTS/readme_xml/readme_81042600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The aim of this programme is to obtain high-resolution and high S/N spectra
of 2 extremely metal-poor stars using the very good sensitivity of UVES in the UV.
We will use these spectra to measure abundances of intermediate-mass neutron-capture
elements in order to confirm the existence of the so-called "weak" r-process.
There are no priorities for the OBs and no time constraints, ie OBs may be executed
at any time. Since the OBs are longer than 1 hour, we are aware that they will not
be repeated if the weather classification changes after the first hour.
We did not submit any finding charts because the targets are very easy to identify
(brightest object in the center of the UVES field of view).
Waiver Requests
A waiver request was accepted on 2008-01-31 for OBs exceeding 1hr (WaiverID:
081.D-0426A.01), with the usual restriction that if the conditions degrade in violation
of the constraints after the first hour, the OB will not be repeated.
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 15:40:24 2009
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