README web version of /home/usg/OPS/MTS/readme_xml/readme_77012600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Primitive Dust in Oort Cloud Comet C/2004 B1 (LINEAR)
Run A: EMMI imaging
This is a simple point-and-shoot imaging program on a comet, a moving target. Saturation
of the coma center must be avoided. Template offsets return comet to approx. start
pixel position. For aborts: repeat complete template.
IMPORTANT: The OB MOV_C2004B1_astrometry" should be taken before 9 April; the data
should be made available to the PI immediately. The two OBs MOV_C2004B1_BVRI_night1/2
are to be executed in two different nights.
For the comet position only approx. RADEC coordinates typical for the expected observing
period (Apr. 2006) are given in the OBs, the differential velocity is set to 0.
Both parameter sets need to be updated by the SM observer before execution of the
OB. The rotator angle remains unchanged (0deg).
Here is a brief cookbook instruction for the OB execution:
- select OB to be executed
- open attached ephemeris file
- enter RADEC coordinates for epoch closest in time to start of OB (ephemeris columns
RA and DEC)
- enter differential RADEC velocity for epoch closest in time to start of OB (ephemeris
columns Vel_RA and Vel_DEC)
- do not change rotator angle of the OB
- start OB
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
The OB MOV_C2004B1_astrometry should be executed before 9 April 2006 and
the data should be released to the PI immediately, since they are required to prepare
Spitzer follow-up observations scheduled for mid May 2006 (submission deadline for
Spitzer is 10 April 2006).
The OBs MOV_C2004_night1/2 should be performed in two different nights in February
to April 2006.
Special Execution Requirements
The central part of the coma must not be overexposed. Since comets are
notoriously unpredictable in their brightness, we can't guarantee for sure that
the carefully chosen integration times in the OBs will be safe against saturation
of the cometary coma. If saturation occurs, feel free to shorten the integration
time appropriately.
Please execute only one OB MOV_C2004B1_night1/2 per night!
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 ?
Last creation of page: Tue Oct 6 15:40:12 2009
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