README web version of /home/usg/OPS/MTS/readme_xml/readme_77066000

Principal Investigator Email Address

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fcomeron@eso.org
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Estimated Total Execution Time (hours, including overheads)

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9:56
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General Description

This run aims at obtaining broad-band (JHKsL') and narrowband (2.12, 2.17
 microns) imaging of the cluster embedded in the HII region IRAS16362-4845. Given
 the colors of the objects of interest, the goal is to reach deep in J and to have
 a good dynamic range in H, Ks. The dichroic and readout modes have been chosen accordingly.
 The L' band imaging is done using normal jitter, rather than chopping and nodding.
 The L27 camera (as opposed to the S54 camera used for shorter wavelenght imaging)
 is used in LW.

The field is pervaded by bright nebulosity and it is thus necessary to take separate
 sky exposures, hence the use of the AutoJitter_Offset template.

The reference star is the brightest star in the cluster, which lies at the center
 of the field to be imaged, and has Ks=8.356. It is also the brightest star in the
 field. Should this star prove unsuitable, two backup stars with magnitudes 9.074
 and 9.529 respectively are also provided. 

Moderate saturation for the brightest stars in the field is not a problem. 

Please note the higher priority of the broad-band images. If possible, execute the
 narrow-band imaging only after the broad-band part has been completed.

Waiver Requests

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No Waiver Request was submitted
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Critical Observing Condition Constraints

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None
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Time-Critical Aspects

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None
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Special Execution Requirements

None, other than the two sets of priorities (1 for broad-band, 2 for narrow-band)
 given in the General Description.

Special Calibration Information

None. Calibration plan is all right. Photometric conditions are not needed,
 as magnitudes of reference stars in the field are already available.

ToO Information

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ToO Activators List

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Is this a Pre-imaging run ?

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false
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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 ?

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N/A
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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 ?

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N/A
```

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

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N/A
```

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

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N/A
```

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 ?

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N/A
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If you have PSF reference star OBs, do the names of those OBs begin with PSF_ ?

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N/A
```

If there are Finding Charts attached to your OBs, is the field-of-view of at least one of these charts 2' x 2' (with clearly labelled field orientation) ?

Have you clearly marked and labelled your wavefront reference objects R1, R2, R3, ... (as specified in the NAOS Preparation Software) on your Finding Charts ?

Have you specified the magnitude of the brightest object in the field-of-view for each OB ?

Are there objects in any of your fields (including standard stars) which are brighter than the limits specified in the User Manual and on NACO web Pages ?

If the previous answer is yes, have you given a list of OBs and a justification for the brightness limit violation in the general description field ?

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N/A
```

Last creation of page: Tue Oct 6 15:40:13 2009
If you have comments, please contact usd-help@eso.org