README web version of /home/usg/OPS/MTS/readme_xml/readme_78505301
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
MIDI observations of the Nova V1280 Sco that suddenly fade in visible
due to the formation of an important of dust within the ejecta.
The calibrator, HD150798, is bright (~100 Jy) and was chosen for its right ascension
which is the same than the Nova, despite a low declibation (-69). This should ease
the scheduling, considering that the two brigthest calibrator are 2h after and 1h30
after the Nova.
The position of the nova should be accurate enough for the acquition. Its visual
magnitude is now close to 11.5, at the center of the finding chart, hopefully bright
enough to avoid a guiding star.
Final note: the MIDI brightness is difficult to evaluate from the K band current
magnitude.
It should be close to the sensitivity limit. Since the dust is warm, the best acquisition
filter is 8.7 micron.
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 ?
Did you indicate for each science star OB the corresponding calibrator
star OB (and vice versa) in the 'Instrument Comments' field ?
Did you check that your chosen calibrator is bright enough for the instrument
mode used ?
If you use calibrator stars which are not in the CalVin database, did
you specify their characteristics in the README file and in the OBs ?
Last creation of page: Tue Oct 6 15:40:17 2009
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