README web version of /home/usg/OPS/MTS/readme_xml/readme_83045205
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
These VISIR images are to support our MIDI observations, which have been
carried out in visitor mode on 7-12 May 2009. Goals are (1) to obtain accurate photometry
at 8.5 and 12 um to back-up (rather inaccurate) photometry with MIDI (to better
calibrate MIDI visibility); (2) to check if there is any extended emission in the
mid-IR for one target (NGC4151), by comparing the image with a PSF star image. Thus,
for NGC4151, we request to observe a PSF star right after the target. The PSF/flux-standard
star HD120933 is chosen so that if NGC4151 is observed at around meridian (note
the very north position, altitude only 26deg), HD120933 will be also at a very similar
airmass (about 2.4). Each science target is the brightest object in the instrument
field.
As of 4 Aug 2009, the last target H0557-385 is now getting observable again toward
the end of the night.
Seeing constraints have been relaxed, compared to the original values.
Waiver Requests
Critical Observing Condition Constraints
One of the targets, NGC4151, is at a very northern position (decilination
+39deg). It will be above the telescope pointing limit for 3 hours, giving an additional
timing contraint. The PSF/flux calibrator for this target, HD120933, is also at
a similar, very northern position.
Time-Critical Aspects
Please execute CAL_PSF_NGC4151_VISIR right after NGC4151_VISIR. It is
preferable if NGC4151 is observed close to the meridian. Then
the PSF/flux-calibrator HD120933, if observed right after NGC4151, will have a similar
airmass to that of NGC4151.
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 the provided finding chart is at a different wavelength than the observations,
did you clearly describe in the README file how to identify the target?
Did you specify a guide star brighter than V=12mag within a field of
r=5arcmin around the science target?
Last creation of page: Tue Oct 6 15:40:29 2009
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