README web version of /home/usg/OPS/MTS/readme_xml/readme_77064600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We propose to observe the quasar PKS 1448-232 (z=2.208; V=16.9) with UVES
at very high resolution (R sim 75,000) in order to study the fine structure in the
absorption lines of intervening OVI and CIV systems. The main goal of this project
is to investigate those OVI and CIV absorbers that are intrinsically narrow, with
Doppler parameters (b-values) less than about 7 km s-1. These systems are not resolved
in currently existing intermediate-resolution UVES spectra. With these new UVES
data we will be able to accurately measure the component structure and line widths
of the intervening OVI and CIV absorbers towards PKS 1448-232. Only these new data
will allow us to derive reliable line-width temperature constraints and OVI/CIV
column density ratios. These parameters are crucial to unveil the mechanisms that
ionize the intergalactic medium at z approx 2.
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 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 15:40:13 2009
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