README web version of /home/usg/OPS/MTS/readme_xml/readme_76046000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is an easy near-infrared imaging programme which use ISAAC capabilities.
The final aim of the programme is the caracterization of the preMS in the SMC star
cluster NGC 346, and the determination of the circummstellar discks frequency around
these sources.
Our proposed nearIR study will also reveal a new generation of stars forming in
the Bok globules surrounding NGC 346.
Three ISAAC set-ups are used for observations in Js, H, and Ks bands. For each band
four different pointing are necesary to cover the entire region. A total of 15 OBs
with an overall execution time of 14 hours have been submitted.
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 15:40:10 2009
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