README web version of /home/usg/OPS/MTS/readme_xml/readme_75047300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a simple high resolution spectroscopy program for bright HB stars.
While some of the objects are flux standards themselves, the standard
calibration plan as specified by ESO for FEROS is sufficient. Given the
brightness of the objects (the target stars are the brightest objects in
the circle drawn at the centre of each finder chart) and the low constraints,
it is an ideal FILLER PROGRAM!
Waiver Requests
Critical Observing Condition Constraints
The OBs from this program can be executed under almost any
ambient conditions. Exposure times within the OBs have been
calculated for a seeing of 2", making sure that no saturation
will occur even at seeing <0.8" (i.e. no slit losses due to seeing)
However since all estimations were made using the FEROS ETC rather than
experience, we would like the observer to check for saturation effects
in conditions of good seeing. We can tolerate thin cirrus; thick cirrus
will probably result in a too big drop of S/N.
Time-Critical Aspects
Special Execution Requirements
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 ?
Did you set 'New Preset' flag in all acquisition templates to 'True'?
If you use any lamp, did you check that it should never be left on at
the end of any OB?
Last creation of page: Tue Oct 6 15:40:07 2009
If you have comments, please contact usd-help@eso.org