README web version of /home/usg/OPS/MTS/readme_xml/readme_83032400

Principal Investigator Email Address

```
mzoccali@astro.puc.cl
```

Estimated Total Execution Time (hours, including overheads)

```
25:00
```

General Description

This is a programme to acquire GIRAFFE HR spectra of disk red clump
stars at different distances (magnitudes) along the line of sight of
two bulge fields. GIRAFFE fibres are thus allocated to stars with
V=12-16. The S/N quoted in the OB comments refers to the faintest ones.
Simultaneous UVES fibres are allocated to peculiar lithium rich stars 
already observed at lower resolution in these fields.
Both fields are rather reddened, thus R magnitudes are >1 mag brighter
than V mag (but not available to us, hence we quote V mag).

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

```
none
```

Time-Critical Aspects

```
none
```

Special Execution Requirements

No special execution requirements were mentioned in the PhaseI.
In the meantime, however, binarity has been suggested as possible 
origin for the Li-rich stars observed with UVES. Having the OBs
of the same field observed in different days would help constraining 
variations in radial velocity, hence binarities.

This is not a strong requirement.
It would be helpful if it does not compromise the programme completion.

Special Calibration Information

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ToO Information

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ToO Activators List

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Do all your OBs comply with the instrument-specific requirements listed on the instrument-specific Phase 2 web page ?

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 ?

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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 ?

```
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
```

Did you specify in your OBs the hour angle range for which your Target Setup files are valid ?

Did you specify in your OBs the magnitudes of FACBs and Guide Star for all your fields ?

Are the FACBs and Guide Star in the brightness ranges specified in the FLAMES manual ?

Did you enter the expected signal to noise in your OBs ?

Last creation of page: Tue Oct 6 15:40:29 2009
If you have comments, please contact usd-help@eso.org