README web version of /home/usg/OPS/MTS/readme_xml/readme_79072200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a prgram to obtain HK spectra of canidate cluster members to measure
the strength of CO bandhead absorption in order to determine whether they are RSGs
or not. Very
low resolution K band spectra already indicate that CO band head absorption is present
but blending prevents the accurate measurement of it's strength, and hence a luminosity
classification. Therefore, even a few (2-3) spectra would be invaluable
in callibrating the lower resolution data. Finally, all sources are very bright
and so the project may be attempted in relatively poor conditions.
For a number of OBs I have been able to place two target stars in each slit - in
each case I have specified in the OB which of the 2 targets in the slit the co-ordinates
correspond to and also the distance in arcsec between the two stars - in no cases
does this match the values selected for the nod throw (60 arcsec) - I hope that
this will keep both stars in the slit at all times.
Note that I was advised to set combined offset=true for these OBs - I hope I have
done this correctly!
Waiver Requests
Critical Observing Condition Constraints
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 ?
Last creation of page: Tue Oct 6 15:40:20 2009
If you have comments, please contact usd-help@eso.org