README web version of /home/usg/OPS/MTS/readme_xml/readme_82008700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our single science target is a z_em=2.831 QSO with magnitude about 17.4
in V. There is a damped Lyman alpha system at z_abs=2.811 which is known to contain
molecular hydrogen. Our primary goal is to obtain high S/N spectra between 350 and
450nm to cover the molecular hydrogen absorption lines.
The science object transits near vertical over Paranal. Please avoid executing OB
during transit; that is, please execute at least 1 hour before transit or any time
after transit.
Each OB is essentially the same: all OBs use dichroic 1 and they all contain an
attached ThAr wavelength calibration template. Half the OBs use the 390+564nm setting,
the other half use the 390+580nm setting.
Over the past decade, this object's brightness has changed from time to time by
about 0.5mag in V. Therefore, it is possible that the object is a little fainter
(or brighter) than used to calculate the S/N at 500nm in the Instrument Comments
field in each OB.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
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 specified the S/N ratio at given wavelength in the User Comments
field of each OB?
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 15:40:26 2009
If you have comments, please contact usd-help@eso.org