README web version of /home/usg/OPS/MTS/readme_xml/readme_83009201

Principal Investigator Email Address

```
Estelle.Moraux@obs.ujf-grenoble.fr
```

Estimated Total Execution Time (hours, including overheads)

```
28:29:18.000
```

General Description

This run consists of SWS-LR spectroscopy using slit central wavelengths
 of 1.65 and 2.2micron. In the 'User Comments' field, indications are given to facilitate
 the target acquisition. The position of the science target in the slit is indicated
 in the Finding Charts of all the OBs. For most cases (all, except 2 OBs where this
 is clearly stated) the target should be centred on the slit.

For spectroscopy at 1.65microns (H-band), all the targets are fainter than >17mag.
 Target acquisition is therefore usually done in the K-filter, where these objects
 are brighter. Whenever possible, a brighter reference star is placed in the slit
 together with the science target to help control the target's position on the spectral
 image. This is always indicated in the Finding Chart and also in the 'User Comments'
 field.

For some targets, due to the existence of bright stars in the FOV, the acquisition
 is done in the NB_2.19 filter using a reference star. The science target is always
 in the slit together with the reference object, but won't be seen in the Narrow
 band filter. The offsets needed to move the Science Target to the centre of the
 slit are provided using the option "Alpha/Delta Offset from Ref. Star". All the
 offsets are less than 1' and always along the slit. For those OBs, 2 finding charts
 are provided, indicating the acquisition image and the positioning of the slit after
 the offset has been applied.

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

```
Does not apply.
```

Time-Critical Aspects

```
Does not apply.
```

Special Execution Requirements

```
Does not apply.
```

Special Calibration Information

```
Does not apply.
```

ToO Information

```
Does not apply.
```

ToO Activators List

```
Does not apply.
```

Is this a Pre-imaging run ?

```
false
```

Pre-imaging Requirements

```
Does not apply.
```

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 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
```

If you are doing spectroscopy, did you draw the slit on the Finding Charts ?

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 15:40:28 2009
If you have comments, please contact usd-help@eso.org