README web version of /home/usg/OPS/MTS/readme_xml/readme_82074001
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
- JHKs imaging of comet 67P/CG, target of the Rosetta Mission.
- This program should be execute as close as possible with the other program 82.C-0740(A),
for VRI imaging & spectroscopy with FORS2.
- This program consists of three sets of OBs, (MOV_67P_JHKs_Oct_1 and MOV_67P_KsHJ_Oct_1
for the first set, same with _2 the second set, and _3 for the third) THAT SHOULD
NOT BE EXECUTED ON THE SAME NIGHT, but likely on three succesive nights, to check
comet variability.
- The three ISAAc programs 082.C-0740(B), (D), and (F) should be executed at about
on month of time distance. Best period for each one is the 2nd half of the month,
if possible.
_ Please insert appropriate coordinates & proprer motion of the Comet, as given
in the ephemeris file. The comet coordinates given in the OB are approximate one,
to be used only for scheduling!
- Since comets are often unpredictable, PLEASE check that photometric center is
not saturated.
Waiver Requests
Critical Observing Condition Constraints
This program should be executed in parallel (or ss close as possible)
with program 082.C-0740(A) at FORS2.
In principle the observations should be:
- First night (thin): execute MOV_67P_JHKs_Oct_1, MOV_67P_KsHJ_Oct_1
- Second night (thin, close to the first one as much a possible): execute MOV_67P_JHKs_Oct_2,
MOV_67P_KsHJ_Oct_2
- Third night (thin, close to the second one as much as possible): execute MOV_67P_JHKs_Oct_3,
MOV_67P_KsHJ_Oct_3
Time-Critical Aspects
This program should be executed in parallel (or ss close as possible)
with program 381.C-0123(A) at FORS2.
The 3 set of OBs (_1, _2 and _3) should be executed possibly during three consecutive
nights. NOT on the same night. See Critical Observing Condition Constrains.
- The three ISAAc programs 082.C-0740(B), (D), and (F) should be executed at about
on month of time distance. Best period for each one is the 2nd half of the month,
if possible.
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 submitted OBs for standard stars, did you use the provided StandardStar
templates ?
If you are using a specific offset pattern or position angle, did you
check carefully the definition in the manual ?
If you are doing spectroscopy, did you draw the slit on the Finding Charts
?
Did you enter the magnitude of the brightest star in the field-of-view
in the 'Instrument Comments' field of each OB ?
If you use the MoveToPixel acquisition, have you given clear instructions
on the FC and in the OB comment section as to how the field should be centered ?
Last creation of page: Tue Oct 6 15:40:27 2009
If you have comments, please contact usd-help@eso.org