README web version of /home/usg/OPS/MTS/readme_xml/readme_81045701
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
V393 Sco has good observability during all semester (April-September,
more than 180 days, about 70% of the long period). We ask for three sub-runs each
12 days long (one OB per night) repeated every two months (April-May, Jun-July,
August-September). With that schedule we can obtain optimal data for science, mapping
well orbital and long-cycle changes in the binary. Accordingly, OB time intervals
have been separated in three two-month blocks, but please keep in mind that consecutive
observations (ONE OB PER NIGHT) are required during each of these three blocks.
Some questions posted by the staff of the User Support Department (Ferdinando Patat)
regarding time critical aspects are replied below:
We propose a minimum time separation between chunks
of 2 weeks and each chunk at least one week long.
Ideally, once a chunk is started, the 12 OBs that are included
must be executed at a rate of one per day during 12 subsequent
nights.
In the case of interruption of a sequence by any reason,
the sequence can be re-started at any time in the 2-month window,
but hopefully as soon as possible.
In the case that the service mode runs last less than
12 consecutive nights, we propose to continue with the
sequence when the new service mode run starts. Each chunk
should be at least one week long, ideally.
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 specified the S/N ratio at given wavelength in the User Comments
field of each OB?
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 you need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:24 2009
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