README web version of /home/usg/OPS/MTS/readme_xml/readme_83060400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We are observing 3 BAL QSO's. Our analysis processes require high spectral
resolution and high signal-to-noise ratios, which are outlined in the Instrument
Comments (note that this is S/N per 2760s observation). We also require telluric
standard stars that will allow us to carefully remove the absorption bands from
our science spectra (outlined in Special Execution Requirements, and User Comments
in the OBs).
Waiver Requests
We submitted a Waiver Request for 083.B-0604(A) on 02/02/2009 to require
that our telluric OBs be executed immediately following our science OBs. The Waiver
was approved on 02/03/2009. We have included the exposure time and overhead associated
with the telluric OBs in our total time calculations, and included instructions
of execution in the Special Execution Requests section of this README.
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
We require telluric standard star observations that correspond to each
science target observation. Thus 1 observing block for the science target and 1
observing block for the telluric standard must be executed consecutively (e.g. the
OB SDSSJ0935+0924-1 followed by OB CAL_0935Tell-D1-1). These are specified in the
User Comments for the OBs. In the event that 2 science OBs are executed consecutively,
only 1 telluric OB needs to be executed. We request that the additional time maybe
be split between the two science OBs as additional exposure time.
Special Calibration Information
Our spectra require telluric calibration spectra from standard stars,
as approved via Waiver. We have included the additional overhead time into our science
observations, and request that the telluric standard OBs be placed consecutively
following our science OBs.
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 15:40:30 2009
If you have comments, please contact usd-help@eso.org