README web version of /home/usg/OPS/MTS/readme_xml/readme_80041700

Principal Investigator Email Address

```
diego@das.uchile.cl
```

Estimated Total Execution Time (hours, including overheads)

```
9.98
```

General Description

Direct imaging of two embedded sources, L1551ne and SSV63, in KLM using
the IR WFS. We have included a Av=20mag in the aocfg files.

--> K & L-band obs. will be performed with AutoJitter.

--> M-band obs.  will be performed chopping and nodding.
WE have checked that the AO configuration includes a sampling 
frequency of, at least, 100 Hz

In the case of SSV63, the field must be centered between the two brightest
stars in the field, as shown in the finding chart.

A PSF-calibrator should be observed after each science exposure.

The targets are the reference objects themselves. They are the brightest 
objects in the FOV. Their magnitudes in the K-band are: 
SSV63: 11.1 mag
L1551ne: 11.4 mag

Although it is not a must, we would appreciate if the targets could be observed
 at the smallest 
possible airmass.

Waiver Requests

080.C-0417A.01.WAV: A Waiver was submitted to execute OBs longer than
 1 hour.
Accepted on 20.07.2007.

Critical Observing Condition Constraints

```
N/A
```

Time-Critical Aspects

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N/A
```

Special Execution Requirements

For the OBs SSV63K, SSV63L, SSV63M:
The center of the FOV must lie between the two brightest
stars in the field (see Finding Chart).

Special Calibration Information

A PSF-calibrator shoud be observed after each science exposure.
We have provided the OBs.

ToO Information

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N/A
```

ToO Activators List

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N/A
```

Is this a Pre-imaging run ?

```
false
```

Pre-imaging Requirements

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N/A
```

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 ?

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 ?

```
N/A
```

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?

```
N/A
```

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

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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 ?

```
N/A
```

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

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 ?

```
N/A
```

Last creation of page: Tue Oct 6 15:40:21 2009
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