README web version of /home/usg/OPS/MTS/readme_xml/readme_82084100

Principal Investigator Email Address

```
heber@sternwarte.uni-erlangen.de
```

Estimated Total Execution Time (hours, including overheads)

```
3.0
```

General Description

The primary target PG1232-136 (Priority: 1) has to be observed BEFORE
 the secondary target WD1055-072 (priority: 2), which will be used to improve the
 spctrum normalisation.
 
We use a small slit (0.4 arcsec) to obtain high resolution. The seeing and transparancy
  is constrained to reduce photon losses to 0.7 arcsec and thin cirrus. 
If transparency, however, is good, a somewhat poorer seeing is tolerable!
Each OB of PG1232-136 contains a series of short exposures, because the radial velocity
 of the star is variable. Seeinging variations during the execution of the OBs are
  not critical!

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

We use a small slit (0.4 arcsec) to obtain high resolution. The seeing
 and transparancy  is constrained to reduce photon losses to 0.7 arcsec and thin
 cirrus. 
If transparency, however, is good, a somewhat poorer seeing is tolerable!
Each OB of PG1232-136 contains a series of short exposures, because the radial velocity
 of the star is variable. Seeinging variations during the execution of the OBs are
 not critical!

Time-Critical Aspects

```
none
```

Special Execution Requirements

```
None
```

Special Calibration Information

```
None
```

ToO Information

```
None
```

ToO Activators List

```
None
```

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 specified the S/N ratio at given wavelength in the User Comments field of each OB?

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 need secondary guiding, are there suitable objects within 30 arcsec from your target ?

```
N/A
```

Last creation of page: Tue Oct 6 15:40:28 2009
If you have comments, please contact usd-help@eso.org