README web version of /home/usg/OPS/MTS/readme_xml/readme_81048502
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is an imaging program with HAWK-I using a NB filter (NB 1.06 micron).
There are two fields, A1689 and CFHT-LS D4. Having as low background as possible
is important, therefore the constraints on the Moon. It is important that these
observations not be executed too close to a Full Moon. Keeping a distance to the
Moon > 50 degrees is highly desirable. The Moon constraints can however be slightly
relaxed if this helps to complete the program.
There are also a few science OBs of the same fields using a broad band filter (J,
Ks). These OBs are important for the programme to provide reference images in the
broad band filters, allowing color selection of the objects detected in the NB images.
Ideally these OBs should be executed in photometric conditions. They have higher
priority than the last NB OBs of a given field.
Ideally, the NB science OBs for A1689 (not for CFHT-LS D4) should be excecuted over
the largest possible time interval, because this field was not observed at all in
P81, and, together with the P81 OBs carried over, it should now be observed entirely
in P83. The reason is to eliminate possible contamination by supernovae: the longer
the time span, the higher the brightness variation and the easier it is to remove.
There are two calibration OBs using the NB filter which is not supported by the
calibration plan. While accurate photometry is not critical to the programme, we
do need reasonable photometric calibration. These OBs need to be executed in photometric
conditions. They do not need to be executed together with the science OBs.
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 ?
Did you enter the magnitude of the brightest star in the field-of-view
in the 'Instrument Comments' field of 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 15:40:24 2009
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