README web version of /home/usg/OPS/MTS/readme_xml/readme_76037200

Principal Investigator Email Address

```
cfaure@astro.puc.cl
```

Estimated Total Execution Time (hours, including overheads)

```
4.8h
```

General Description

K-band integral field spectroscopy of young embedded clusters in the starbursting
 environment of the AGN in NGC1365. AO loop closed on the nucleus (AGN). The idea
 is to resolve and detail the brightness and velocity distribution of nebular lines
 around the embedded clusters. 

The reference (central AGN) is quite faint, at the limit for closing the loop, hence
 the program needs good seeing. Each observation was split into two similar OBs for
 two reasons:
-the OBs would be larger than 1h if they were in one block
-we can have better benefit of the periods of good seeing.

The targets emit continua at a level of about 1mJy in the K band corresponding to
 a K magnitude of 14.5. Each targets is composed of a non-resolved source (on the
 ISAAC image diam<0.6arcsec) surrounded by extended emission up to distance of
 ~2arcsec from the core.

On the finding charts for the source called M4, the fiels should be centered as
 drawn i.e., the centered on the N-band cluster, which is slightly offset with respect
 to the integrated K band light.

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

Since the AGN used to close the loop is rather faint (R=15.4 and B-R=1.6),
 the weather constraint, especially the seeing (<0.6) are essential.

Time-Critical Aspects

```
No time critical aspects
```

Special Execution Requirements

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Special Calibration Information

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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 ?

```
N/A
```

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

```
N/A
```

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 ?

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
```

Did you indicate the magnitude of the brightest object in the field in each SINFONI OB?

```
N/A
```

If you are using the AO: Did you indicate for every OB the magnitude of the guide star, and its distance to the target (if any)?

```
N/A
```

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

```
N/A
```

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

```
N/A
```

Did you make really sure that none of your OBs ever saturates the detector?

If you are using the AO: did you enter the correct Strehl Ratio (on-axis, K-band) AND the seeing value in the constraint set?

Last creation of page: Tue Oct 6 15:40:10 2009
If you have comments, please contact usd-help@eso.org