README web version of /home/usg/OPS/MTS/readme_xml/readme_80025900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Science
=======
------------------- Please communicate about this program to: lbarrera@umce.cl
(PI) AND tubiana@mps.mpg.de AND boehnhardt@mps.mpg.de! -------------------
Program: 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), 2 OBs to be executed during 20 Sep and 24 Oct 2007) and 2 OBs
during (24 Oct and 15 Nov 2007). Both OBs of each time interval can be executed
either subsequently or one per night. The latter is in particular adviceable for
the second time interval (24 oct to 15 Nov 2007).
- Object visibility: The comet is low in the early evening sky and requires pointing
soon or immediately after end of twilight. It is acceptable to start the OB before
the end of astronomical twilight, i.e. about 10 min before dark sky conditions are
reached (Sun 18 deg below horizon).
- 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.
- 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 time interval when the OBs should 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:
===================================
- select OB for execution (check time constraints)
- 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 no problem, also not vignetting of lower CCD
Waiver Requests
Critical Observing Condition Constraints
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 15:40:21 2009
If you have comments, please contact usd-help@eso.org