README web version of /home/usg/OPS/MTS/readme_xml/readme_79503500
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Imaging and Spectroscopy of Asteroid/Comet Elst-Pizarro, a moving target.
The program asks for RI imaging and LSS spectroscopy of the object. Besides the
two asteroid OBs, a solar analog star is to be observed for calibration purposes.
Run A should be done before Run B.
(1) It is advantageous to perform all OB s during the same night, in particular
the ones for the moving target.
(2) When performing both OBs of the moving target during the same night, it is recommended
to perform the imaging OB of the asteroid before the spectroscopyone.
(3) Before executing the OB on the moving target please enter in the OB
==> RADEC of the asteroid at the epoch closest in time to the expected start
time of the OB
==> the motion rates in RADEC at the epoch closest in time to the expected
start time of the OB
==> the rotator position angle which is "MINUS*PSANG" value in the table
Ephemeris: the attached ephemeris file lists for 15min time tags in UT the RADEC
of the asteroid, its RADEC motion rates, the airmass, the apparent visual magntiude,
the position angle of the tail direction (PSANG).
Finding chart: No finding chart is prepared, instead we provide an image of the
appearance of the asteroid. The motion range of the object is too wide to be reasonably
covered by traditional finding charts and - more important: 1) for imaging the ephemeris
precision is good enough (a few arcsec) to allow accurate pointing and 2) for spectroscopy
the target is easily recognizeable since it has a long and narrow tail (see the
attched image).
Solar analog star calibration: Ideally to be done during same night as the asteroid
spectra. Star is of G2V, 8mag in V.
Waiver Requests
Critical Observing Condition Constraints
Try to execute all OBs during the same night. Since the target is moving,
please before observing enter the coordinates and the proprer motion given in the
attached ephemeris.
Please for the spectroscopy part enter also the angle of the rotator (equal to -
PsAng in the ephemeris) in order to have the tail along the silt.
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 you have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS1 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:20 2009
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