README web version of /home/usg/OPS/MTS/readme_xml/readme_83502000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is the set of observing templates for the VISIR observations of the
dusty nova V1280 Sco.
Given our knowledge, the target is probably brighter than 5Jy in all filters. In
that case, we prefer that the observations to be performed in BURST mode (alternative
283.D-5020(D)), if possible. If not, the following templates should be used.
The calibrator, HD152834, is a M5 star, with a Iras 12micron flux of 8.2Jy. This
flux is similar to the expected flux of V1280 Sco, and above the 5Jy threshold to
allow burst mode observations. Therefore, the same calibrator has been chose for
the VISIR templates A and D.
The VISIR observations are challenging: the source is a 0.3" diameter dusty ring.
Therefore the best spatial resolution is needed to study it (implying good quality
observations, and good PSF data too).
Last note: we are currently not able to check in the alternative templates, 283.D-5020(D),
as they are not offered in service mode. Is a waiver request necessary?
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 15:40:31 2009
If you have comments, please contact usd-help@eso.org