README web version of /home/usg/OPS/MTS/readme_xml/readme_75036100
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a K-band spectroscopic program with 31 targets, with a range of
magnitudes of K=11.5-17. In some OBs there are two targets in the slit, while in
others there is only one target. The slit position angle in each OB varies according
to the requirements of covering both targets (if there are two) and also avoidance
of extraneous stars in the slit. All targets are in the Galactic Centre so the
fields are crowded. We have therefore provided three finder charts for each target
field. The first finder is from 2MASS, showing the full ISAAC field with the required
slit centre position at the centre of the finder. However, our targets are not
always visible on the 2MASS finders due to the low resolution and limiting magnitude
of 2MASS. Therefore the second finder chart is the ISAAC image we obtained for
these target fields in 2003, showing our target(s) and the required slit position.
Tn the case of the full ISAAC finders the required slit centre position is generally
*not* at the centre of the finder image. Finally, the third finder is a zoom-in
from our ISAAC finders with a 40 arcsec^2 size, centred at the required slit centre
and showing the required slit position angle.
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 ?
If you submitted OBs for standard stars, did you use the provided StandardStar
templates ?
If you are using a specific offset pattern or position angle, did you
check carefully the definition in the manual ?
If you are doing spectroscopy, did you draw the slit on the Finding Charts
?
Did you enter the magnitude of the brightest star in the field-of-view
in each OB ?
If you use the MoveToPixel acquisition, have you given clear instructions
on the FC and in the OB comment section as to how the field should be centered ?
Last creation of page: Tue Oct 6 15:40:07 2009
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