README web version of /home/usg/OPS/MTS/readme_xml/readme_78029501
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is an observation of the close environment of the bright and nearby
Be star Achernar in order to search for a compact envelope.
As we are searching for an angularly small envelope, we need a PSF star to be observed
immediately before or after Achernar. For this purpose, we have selected hd9362,
that is a photometric standard for the mid-IR (Cohen et al. 1999 AJ 117, 1864 catalogue).
The two OBs "Achernar" and "PSF-hr9362" should be observed together (the order does
not matter) in order to sample the same seeing conditions. The execution of the
""Achernar" OB takes 1 hour, while the "PSF-hd93262" OB takes 30 minutes. In total,
this means we need 1.5 hour of continuous observations with VISIR.
The two objects are very bright stars, that are easy to acquire with VISIR. In both
cases, they are the brightest and (as far as we know) only object in the VISIR field.
We have selected the "MoveToPixel" acquisition template nevertheless, in order to
have the object properly positioned for the subsequent "perpendicular" chopping-nodding
(our sources are point-like). The amplitude of the chopping amplitude is set to
10".
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 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 15:40:15 2009
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