README web version of /home/usg/OPS/MTS/readme_xml/readme_76079800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The aim of the program is to obtain visibilities on selected asteroids,
and from these to derive the size of the targets. In addition, together with spectrophotometric
information, these data can be used to derive the albedo and possibly to check and
improve the current thermal models.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
The observing date constraints for each target are selected based on the
expected evolution of the correlated flux during the observing period. In general,
the brightness of the target is related to its distance from Earth and therefore
on its size. The visibility tend to decrease when the brightness of the object increases.
Outside of the indicated time limits the target is expected to be too faint or too
resolved to allow successful fringe detection.
HERE ARE REPORTED THE TIME SLOTS FOR EACH TARGET
951 GASPRA 2005-11-01T04:00:00 - 2005-12-15T04:00:00
64 ANGELINA 2005-12-15T07:30:00 - 2006-01-15T10:00:00
234 BARBARA 2005-11-01T02:00:00 - 2005-12-31T10:00:00
21 LUTETIA 2005-11-26T07:00:00 - 2005-12-31T10:00:00
Special Execution Requirements
As described in the proposal, we would like, if at all possible, the two
visibility points for 951 Gaspra (plus calibrator) to be executed one immediately
after the other (i.e. with one hour time difference), in order to make sure that
one of the visibility points is obtained close to the maximum brightness (the rotation
period being 7 hours).
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 ?
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 15:40:11 2009
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