README web version of /home/usg/OPS/MTS/readme_xml/readme_75044501
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
These are 4 imaging runs designed to sample the globular cluster NGC 6809
in B, R and Halpha. One OB uses short exposures to capture the brighter stars of
the cluster, the other OBs use long exposures for the fainter stars. Since crowding
is not an issue for the brighter stars there are taken under moderate seeing constraints,
0.9", whereas the deep OBs need good seeing (0.6" or less). These deep OBs use 1x1
binning to better sample the PSF.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
Three OBs for taking B, R and Halpha flatfields with 1x1 binning are specified.
When the three science OBs using 1x1 binning are taken within two to three days,
flatfields taken on one of these days will suffice. If the science OBs are taken
further apart, please execute the calibration OBs at each night.
No photometric standards need to be observed with 1x1 binning. The standard calibration
plan using 2x2 binning will suffice.
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 have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS2 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:07 2009
If you have comments, please contact usd-help@eso.org