README web version of /home/usg/OPS/MTS/readme_xml/readme_75066800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a pure imaging programme consisting of OBs for SW observations
(Ks, NB_2.12 and NB_2.17)
using the S13 camera and for LW observations (Lp without chopping and Mp with chopping)
using
the L27 camera. Our targets are bright at optical wavelengths, hence, the VIS WFS
is used in
all OBs. The execution of all OBs (even those for Mp with chopping) should be straightforward.
Our targets are also bright at infrared wavelengths. As it is crucial for our scientific
goals
to keep the source intensities in the linear range of the detector, we kindly ask
the nighttime
support astronomer to carefully check the actually measured counts before each science
template
is executed. Should it turn out that the measured counts are in the non-linear range
of the
detector, we kindly ask the nighttime support astronomer to properly adjust the
DIT x NDIT
setting of the science template(s).
To perform accurate data analysis and interpretation, for each science OB we have
submitted a
corresponding PSF reference OB, which should be executed immediately after the science
OB.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
For accurate data analysis and data interpretation purposes, the successful
execution of a science OB
must be followed immediately by the execution of the corresponding OB with the PSF
reference source.
All OBs, both for science targets and PSF reference sources, perform the observations
in two rotator
positions: first, 0 degree and second, 33 degree. After applying the rotator angle
offset, the source
should be (roughly) re-centered in the CONICA field-of-view.
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 have PSF reference star OBs, do the names of those OBs begin with
PSF_ ?
If there are Finding Charts attached to your OBs, is the field-of-view
of at least one of these charts 2' x 2' (with clearly labelled field orientation)
?
Have you clearly marked and labelled your wavefront reference objects
R1, R2, R3, ... (as specified in the NAOS Preparation Software) on your Finding
Charts ?
Have you specified the magnitude of the brightest object in the field-of-view
for each OB ?
Are there objects in any of your fields (including standard stars) which
are brighter than the limits specified in the User Manual and on NACO web Pages
?
If the previous answer is yes, have you given a list of OBs and a justification
for the brightness limit violation in the general description field ?
Last creation of page: Tue Oct 6 15:40:08 2009
If you have comments, please contact usd-help@eso.org