README web version of /home/usg/OPS/MTS/readme_xml/readme_76004100

Principal Investigator Email Address

```
ltacconi@eso.org
```

Estimated Total Execution Time (hours, including overheads)

```
10:06:26.000
```

General Description

1. This program is designed to obtain H and K spectroscopy of two Seyfert
 galaxies (missing from P74), with two         slit positions per galaxy.  In each
 case please be sure to center the nucleus on the slit.  This is especially
   important for the NGC1097 observations, as the starformation ring in this system
 is not much smaller than the 
   array.  NOTE, the Position Angle for NGC1097 slit #2 is a good starting point
 only!  Please adjust the 
   position angle as required to ensure that the slit passes both through the nucleus
 and through the bright   
   ring-knot to the NW of the nucleus.

2. In addition, wherever possible, please complete a series before going on to the
 next.  For example, choose   
   NGC1097_H_slit_1.3_of_3 over NGC1097_H_slit_2.1_of_3.

3. If the chosen DIT values result in saturation (not anticipated) please do adjust
 the DITs such that the
   data lie just below the non-linearity limit.  In every case the brightest source
 in the field is the nucleus 
   of the galaxy itself, and both NGC1097 and NGC1386 are K = 12.2 in 1" (determined
 from NACO SV observations).

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

```
none
```

Time-Critical Aspects

```
none
```

Special Execution Requirements

```
none
```

Special Calibration Information

```
none
```

ToO Information

```
N.A.
```

ToO Activators List

```
N.A.
```

Is this a Pre-imaging run ?

```
false
```

Pre-imaging Requirements

```
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 ?

```
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 ?

```
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_ ?

```
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 ?

```
N/A
```

Last creation of page: Tue Oct 6 15:40:09 2009
If you have comments, please contact usd-help@eso.org