README web version of /home/usg/OPS/MTS/readme_xml/readme_78018500
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
High Resolution Spectroscopy of a bright QSO with z_em = 2.785
Of particular interest are absorption lines in a damped Lyman
system at z_abs = 2.61844, especially at the UV end of the spectrum,
shortwards of 3500 A.
Two standard settings have been chosen 390+564 (Dic-1) and 390+760 (Dic-2)
to cover most of the optical spectrum at relatively uniform S/N. (S/N will
be lower in the far-UV). 6 OBs prepared at each setting.
QSO should be visible at acquisition.
All the observations are to be conducted with the slit vertical
on the sky (throughput in the UV is critical).
Waiver Requests
For maximum observing efficiency and compatibility with earlier
archive data on the same object, we chose exposure times of 3800-3900 s,
leading to execution times of about 1 hour and 15 minutes.
These longer exposures were approved by USD. I am aware that
these extended exposure time mean that ESO cannot guarantee
that the observing condition requirements are maintained throughout
the full exposure time.
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 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 15:40:15 2009
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