README web version of /home/usg/OPS/MTS/readme_xml/readme_78003601

Principal Investigator Email Address

• antonella.barucci@obspm.fr

Estimated Total Execution Time (hours, including overheads)

• 02:13:10

General Description

• Photometry and spectroscopy of moving target (check the ephemeris).  Each
   science goal is given with a calibrator which must be performed just after or before
   the science OB at the same airmass. We inform that we request simultaneous observations
   between the FORS (176.C-0036(A)), ISAAC (178.C-0036(B)) and SINFONI (178.C-0036(J))
   runs for each object (2000 GN171  and Chariklo). The observation with FORS can confirm
   the good ephemeris of the objects, which is, in general, in the center of FOV. For
   Chariklo we have one photometric and one spectroscopic run (with respectively one
   photometric and one spectroscopic OBs for calibration) in the case of FORS and ISAAC
   runs. For 2000 GN171, we require only photometric observation with ISAAC. Each analog
   star can be used after the observation of Chariklo. We request to the astronomer
   to choose the calibrator with the nearest airmass.

Waiver Requests

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Critical Observing Condition Constraints

• Observe at the lowest airmass (look the constraint set)

Time-Critical Aspects

• The objects must be observed at small airmass between march 15 (00h00
   UT) and 25 (only available period with UT1, UT2 and UT4 simultaneously)

Special Execution Requirements

• We require simultaneous FORS, ISAAC and SINFONI observations and particularly
   to have similar airmass between our science target and the spectroscopic calibration
   targets (solar analogs: SA107998 or HD147935). We give two analog stars. Each analog
   star can be used after the observation of each target. We request to the astronomer
   to choose the calibrator with the nearest airmass

Special Calibration Information

• We give our own calibrators. In the case of spectroscopy, we give solar
   analog Obs and for photometry, standard stars OBs are also given. Our calibration
   Obs must be performed just before or just after our science target.
  SA107998 and HD147935 for spectroscopy
  S860-D for photometry

ToO Information

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ToO Activators List

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Is this a Pre-imaging run ?

• false

Pre-imaging Requirements

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Source(s) of Pre-imaging

• ---(Empty)---

Pre-imaging sources not listed above

• ---(Empty)---

Do all your OBs comply with the instrument-specific requirements listed
 on the instrument-specific Phase 2 web page ?

• YES

If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
 Category for each Observing Template ?

• N/A

Do all your finding charts comply with both the general and instrument-specific
 Phase 2 Web Pages ?

• YES

If you submitted OBs for standard stars, did you specify the magnitude
 and spectral type of all standard stars in the OBs ?

• YES

Have you included OBs for any calibrations that you need but which are
 not part of the Calibration Plan ?

• YES

If you are observing Moving Targets, have you attached suitable ephemeris
 files to your OBs?

• YES

If you have preferences which OBs should be executed first, did you make
 use of the User Priority field in the OBs ?

• N/A

If this is a run that requires coordinated observations with other facilities,
 did you give proper instructions in the Time-Critical Aspects Section ?

• YES

If you submitted OBs for standard stars, did you use the provided StandardStar
 templates ?

• YES

If you are using a specific offset pattern or position angle, did you
 check carefully the definition in the manual ?

• N/A

If you are doing spectroscopy, did you draw the slit on the Finding Charts
 ?

• N/A

Did you enter the magnitude of the brightest star in the field-of-view
 in the 'Instrument Comments' field of each OB ?

• YES

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 ?

• N/A