README web version of /home/usg/OPS/MTS/readme_xml/readme_84102900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We would like slit spectra of 22 elliptical galaxies, 16 of which are
in the Virgo cluster. The observational plan is to abserve the centre of each galaxy
then a sky position, and then repeat these 2 pointings in reverse; ie the classical
O-S-S-O sequence. For the smaller objects this can be achived with the "FixedSkyOffset"
template (max offset is 100"). For the larger objects we implement the same strategy
with the "GenericOffset" template.
The S/N values entered in the OBs refer to the central few pixels.
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 ?
Last creation of page: Tue Oct 6 15:40:32 2009
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