README web version of /home/usg/OPS/MTS/readme_xml/readme_78003616

Principal Investigator Email Address

```
antonella.barucci@obspm.fr
```

Estimated Total Execution Time (hours, including overheads)

```
06:31:15
```

General Description

For each target, we need ISAAC observations close to the FORS2 ones and
 ISAAC simultaneously with SINFONI. Photometry and spectroscopy of moving target
 (check the ephemeris).  Each science goal is given with a calibrator which must
 be performed just after the science OB at the same airmass. We inform that we request
 almost simultaneous observations between the FORS2 (176.C-0036(P)), ISAAC (178.C-0036(Q))
 and SINFONI (178.C-0036(L)) runs for each object. Simultaneous is acceptable within
 few hours (for ISAAC and SINFONI) or few days maximum (for FORS2 and others instruments).
 The observation with FORS2 can confirm the good ephemeris of the science target,
 which is, in general, in the center of FOV. For each object we have one photometric
 and one spectroscopic run (with respectively one photometric and one or several
 spectroscopic OBs for calibration in the case of FORS runs). For SINFONI (176.C-0036(L))
 and ISAAC, we have 1 spectroscopic calibration OB for each science target. 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. For the observations
 with SINFONI, the objects, in general too faint, are not visible after the pre-acquisition
 images (do not loose time to check the finding charts).

Waiver Requests

178.C-0036Q.01.WAV
"We ask to have the possibility to decrease the constraints about the fact that
 NDITxDIT must be >60s"

Critical Observing Condition Constraints

Observe at the lowest airmass (look the constraint set) and only at the
 beginning of the night.

Time-Critical Aspects

Critical periods: do not observe the following targets in the
indicated periods, because of small moon distance/ bright star in the
field of view.

********
2060 Chiron:
NO observations from 17-Oct-2007 20:00 UT to 28-Oct-2007 06:00 UT (moon)
NO observations from 11-Nov-2007 20:00 UT to 27-Nov-2007 06:00 UT (moon + bright
 star)
********

********
120178 (2003 OP32)
NO observations from 02-Oct-2007 20:00 UT to 10-Oct-2007 06:00 UT (bright star)
NO observations from 18-Oct-2007 20:00 UT to 29-Oct-2007 06:00 UT (moon)
NO observations from 01-Nov-2007 20:00 UT to 03-Nov-2007 06:00 UT (bright star)
NO observations from 14-Nov-2007 20:00 UT to 27-Nov-2007 06:00 UT (moon)
********

********
44594 (1999 OX3)
NO observations from 01-Oct-2007 20:00 UT to 05-Oct-2007 06:00 UT (bright star)
NO observations from 07-Oct-2007 20:00 UT to 08-Oct-2007 06:00 UT (bright star)
NO observations from 12-Oct-2007 20:00 UT to 13-Oct-2007 06:00 UT (bright star)
NO observations from 18-Oct-2007 20:00 UT to 28-Oct-2007 06:00 UT (moon)
NO observations from 03-Nov-2007 20:00 UT to 05-Nov-2007 06:00 UT (bright star)
NO observations from 14-Nov-2007 20:00 UT to 27-Nov-2007 06:00 UT (moon)
********

********
73480 (2002 PN34) 
NO observations from 11-Oct-2007 20:00 UT to 12-Oct-2007 06:00 UT (background star)
NO observations from 16-Oct-2007 20:00 UT to 17-Oct-2007 06:00 UT (background star)
NO observations from 19-Oct-2007 20:00 UT to 29-Oct-2007 06:00 UT (moon)
NO observations from 07-Nov-2007 20:00 UT to 08-Nov-2007 06:00 UT (background star)
NO observations from 12-Nov-2007 20:00 UT to 28-Nov-2007 06:00 UT (bright star +
 moon)
********

Special Execution Requirements

We require nearly simultaneous FORS, ISAAC and SINFONI observations. We
 require to have similar airmass between our science target and the calibration target.
 We give one or several analog stars. Each solar analog 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

List of our calibrator for each target. We request to astronomer to choose
 the spectroscopic standard with the nearest airmass is possible 
For 2060: Spectroscopic standard: CAL_LD112_1333 
For 44594: Spectroscopic standard: CAL_HD210078 
For 73480: Spectroscopic standard: CAL_LD115_271
For 120178: Spectroscopic standard: CAL_LD112_1333

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

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Pre-imaging sources not listed above

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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 ?

```
N/A
```

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 ?

```
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 ?

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 ?

```
N/A
```

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 ?

```
N/A
```

Last creation of page: Tue Oct 6 15:40:15 2009
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