README web version of /home/usg/OPS/MTS/readme_xml/readme_79030300
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$)
in order to study the fine structure in the absorption lines of
intervening O\,{\sc vi} and C\,{\sc iv} systems. The main goal
of this project is to investigate those O\,{\sc vi} and C\,{\sc iv} absorbers
that are intrinsically narrow, with Doppler parameters ($b$-values) less than $\sim
7$
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 O\,{\sc vi} and C\,{\sc iv}
absorbers towards PKS\,1448$-$232. Only these new
data will allow us to derive reliable line-width temperature constraints
and O\,{\sc vi}/C\,{\sc iv} column density ratios. These parameters are
crucial to unveil the mechanisms that ionize the intergalactic medium at $z\approx2$.
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 15:40:18 2009
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