README web version of /home/usg/OPS/MTS/readme_xml/readme_80051100
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This run aims at achieving the spatially resolved spectroscopy at low-resolution
of the circumstellar disk of HR 4796 A. The disk is nearly edge-on and its major
axis has a PA of +27 deg from Noth to East (see finding chart). The acquisition
phase place the source at the center of the detector. The long-slit (32" long, 1"
width) must be aligned along the major axis of the disk (+27 deg), and the chopping
and nodding must be executed within the slit. In N, the disk is extended by ~1"
from the star.
The target has a companion at 7" distance (HR 4796 B, see finding chart), but HR
4796A is the brightest source of the region in N.
Finding charts have been added for each OB: at 10 microns HR4796A should be the
brightest star in a 2x2 arcmin FOV
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
No special time critical aspects for this run.
Using the ESO observability tool, we found that, in P80, HR 4796 can be observed
at airmass<1.5 from beginning of January to end of March (end of the period)
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 15:40:21 2009
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