README web version of /home/usg/OPS/MTS/readme_xml/readme_75001800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
General Overview
----------------
High resolution spectroscopy of a R = 19.5 QSO at redshift z = 2.572
Standard UVES setting 390+564 (DIC-1). After low signal has been detected in blue
spectra with our original 3200s integrations (email from 04.10.05), we followed
recommendation by PSO to use exposure times up to 5400s. Therefore, number of remaining
OBs is now reduced to 9 (from 14 that were left), each of them with 5320s integrations.
QSO should be visible at acquisition.
Should the observer experience any difficulties at acquisition,
it is also possible to offset from a nearby star (indicated on the
finding chart).
The coordinates of the offset star are (J2000)
RA: 23:46:25.31
Dec: 12:47:26.83
From this reference star, offset 1.46 arcsec E and 17.04 arcsec N
to reach the QSO.
All the observations are to be conducted with the slit vertical
on the sky
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 15:40:06 2009
If you have comments, please contact usd-help@eso.org