README web version of /home/usg/OPS/MTS/readme_xml/readme_79055600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Waiver Requests
Critical Observing Condition Constraints
They are several visual binaries. If the target cannot be identified with
the help of the finding chart, please, send the SV image.
Although THN is asked, the program can be executed with THK clouds as far as we
get a total S/N around 100-120. In order to achive this S/N in a very bad night,
the night astronomer can increased the exposure time and/or repeat the OB.
Time-Critical Aspects
Special Execution Requirements
In many cases, the FCs don't make any sense (very bright stars). As a
general rule, the target is always the brightest star of the field, except for the
visual binaries HD37551B and HD222259B where the fainter star should be observed.
This is indicated in the respective finding charts.
We have tried as much as possible to look for any ambiguity affecting target identification.
If any problem arises (two stars of same magnitude, for instance). Please, send
us the SV image for clarification.
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 15:40:19 2009
If you have comments, please contact usd-help@eso.org