README web version of /home/usg/OPS/MTS/readme_xml/readme_78506200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is the observation of a Damped Lyman alpha system in front of a faint
quasar.
We aim at high resolution power (R=45 000) and sufficient SNR: in the blue to observe
molecular absorption lines associated to the DLA, and in the red to observe singly
ionized associated metals.
The observation consist in 6 OBs:
-Three identical OBs using setting 390+580 to cover molecular lines in the blue,
some additional molecular and metal lines in the red.
-Three identical OBs using setting 390+610 to covermolecular lines in the blue and
metal lines in the red, uncovered by 390+580.
Waiver Requests
Two Waiver Requests were submitted on March, 16th and accepted on March,
19th.
1) We asked for 1h20 long OBs.
2) We asked for a non-standard setting for 3 OBs: 390+610 with template UVES_dic1_obs_expfree,
to cover some absorption lines (from ZnII and CrII) not observable with 390+580.
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 15:40:17 2009
If you have comments, please contact usd-help@eso.org