README web version of /home/usg/OPS/MTS/readme_xml/readme_80052100

Principal Investigator Email Address

```
kawka@sunstel.asu.cas.cz
```

Estimated Total Execution Time (hours, including overheads)

```
50
```

General Description

The aim of this run is to obtain circular spectropolarimetry for a selected
 high-proper motion white dwarf candidates. The flux spectra will be used to determine
 the spectral type of the star, and if the star is confirmed to be a white dwarf,
 it will be used to determine the atmospheric properties, i.e., chemical composition,
 effective temperature and surface gravity. The circularly polarized spectra will
 be used to determine where the white dwarf is magnetic, and determine its longitudinal
 magnetic field if polarization is detected.

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

We do not have any specific condition constraints, except that we request
 that the fainter targets (V > 17 mag) be observed at grey time or darker. The
 brighter objects (V < 17 mag) can be observed during any lunar phase. The sky
 transparency should be variable/thin cirrus or better.

Time-Critical Aspects

The stars can be observed when conditions are allowed, and he we have
 no time constraints on any of the targest.

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
```

If you have prepared your finding charts with tools other than FIMS, do they comply with the specifications on the FORS1 Phase 2 web page ?

Last creation of page: Tue Oct 6 15:40:21 2009
If you have comments, please contact usd-help@eso.org