README web version of /home/usg/OPS/MTS/readme_xml/readme_80507700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We want to take deep images of a faint comet at aphelion to search for
activity, and to measure the nucleus properties if we find no activity. There are
3 long OBs (waiver requested to have OBs of 1.3 hours duration), one for each of
VRI. Total time 4 hours.
Other than the fact that the target is moving and the exposure times need to be
adjusted based on the ephemeris file (see execution requirements section below)
this is simple VRI imaging. Standard calibrations please.
Note that the ephemeris file has positions, exposure times, total number of exposures,
and an estimate of the expected nucleus magnitude assuming that the comet is inactive.
It has one line every 10 minutes whenever the comet is above the airmass cut off
and the moon is down, but it doesn't move so fast that the position needs to be
updated every 10 minutes. One position at about the midtime of the OB execution
will keep the comet in the FOV.
Waiver Requests
Waiver ID 280.C-5077A.01 submitted to have OBs longer than 1 hour in duration.
Decision pending, but OBs & this readme submitted now anyway to have a chance
of getting the OBs into the queue before this weekend (ie during the dark time in
April). NB the total time on the OBs currently is under 1 hour to allow the p2pp
submission process to work, but each will take 1.3 hours using the exposure times
and number of exposures listed in the ephemeris file.
Critical Observing Condition Constraints
Time-Critical Aspects
ASAP please!
It would be best to do all 3 OBs together, if possible, although obviously that
may be tricky from an operations point of view, and should be seen as a weak constraint.
The OBs should be executed as early in P81 as possible, both from the visibility
of the target and to get the comet as close to aphelion as possible.
Special Execution Requirements
Although this is a moving target, we want to track at the sidereal rate
- do NOT add an additional velocity! This is so we can use the stars to measure
the image PSF and compare the comet PSF to look for faint activity. To do this we
have to keep the exposures short, and these depend on the rate of motion (exposure
times = time for the target to move 0.5"). The ephemeris file lists the position
at each possible time in P81 along with the exposure time and the number of exposures
that will give a total OB of 1.3 hours at that epoch. PLEASE UPDATE THE EXPOSURE
TIME AND NUMBER OF TELESCOPE OFFSETS as well as the RA & DEC position to the
values listed in the ephemeris file at execution time. Note that the OB is set up
to continue looping around 4 jitter positions for the total number of exposures
(= number of offset positions), so there is no need to update the list of offset
positions - p2pp will automatically repeat from the start of the list.
Please also check the first few images to make sure that the comet is not too close
to any bright stars.
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 15:40:23 2009
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