README web version of /home/usg/OPS/MTS/readme_xml/readme_79068701
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Science
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Please communicate about this program to: lbarrera@umce.cl (PI) AND tubiana@mps.mpg.de
AND boehnhardt@mps.mpg.de!
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R filter imaging of the ROSETTA target comet 67P/Churyumov-Gerasimenko to monitor
the dust environment of the comet while it is approaching the Sun. The main goal
of the monitoring is the detection of distant activity of the comet.
In principle a simple point-and-shoot program on a MOVING TARGET. It is a sequence
of 4 OBS (0.33h/OB), to be executed one per month in April (MOV_67P_monitoring_17April),
June (MOV_67P_monitoring_15June), August ( MOV_67P_monitoring_15August) and September
(MOV_67P_monitoring_15September).
Special note: large offsetting amplitudes at the beginning of the science template
(change of guidestar is ok, also guide probe vignetting of the lower CCD). Do not
worry about the field crowdiness, observations happen close to the galactic plane.
IMPORTANT NOTES
===============
April:
On April 17 Spitzer will perform spectroscopy of the comet. If possible, we require
to execute the OB (MOV_67P_monitoring_17April) simulataneous with Spitzer observations
or at least as close as possible in time.
The Spitzer window is scheduled for
April 17 4:20-5:50UT.
In June, August and Septemebr no time constrain is required.
- Blind acquisition, i.e. object identification is not necessary, though easily
possible (by blinking). Please check telescope pointing through DSS image!
- The OB names contain the month when the OBs have to be executed.
- Ephemeris provides in 10min time steps for the daily visiblity window of the comet
at Paranal
* RADEC positions (hh mm ss.ss, sdd mm ss.s)
* RADEC velocities (arcsec/s)
* Airmass
* Vis. Brightness (mag)
* distance comet-moon TOM (deg)
* moon phase (%)
Cook instructions for OB execution:
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- select OB for execution (the one relative to the right month)
- check requirement for environmental conditions (CLR, moon phase/distance)
- in OB enter RA and DEC from target ephemeris (fields RA and DEC) that are closest
in time to the expected start time of the OB
- in OB enter differential velocity in RA and DEC (fields VEL_RA and VEL_DEC) from
target ephemeris that are closest in time to the expected start time of the OB
- perform preset and start R filter offset exposures
- change of guide star is not a problem, also not vignetting of lower CCD
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
April:
On April 17 Spitzer will perform spectroscopy of the comet. If possible, we require
to execute the OB (MOV_67P_monitoring_17April) simulataneous with Spitzer observations
or at least as close as possible in time.
The Spitzer window is scheduled for
April 17 4:20-5:50UT.
In June, August and Septemebr no time constrain is required.
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 15:40:19 2009
If you have comments, please contact usd-help@eso.org