README web version of /home/usg/OPS/MTS/readme_xml/readme_78073400

Principal Investigator Email Address

```
gajh@st-andrews.ac.uk
```

Estimated Total Execution Time (hours, including overheads)

```
02:59:10
```

General Description

This programme will obtain high resolution spectra of T Tauri stars in
 the Orion Nebula Cluster in order to measure their spectral types and measure spectral
 broadening due to rotation. Using results from a recent X-ray survey of these same
 stars we will establish how X-ray emission from these stars depends on rotation
 rate and spectral type, thus testing the model put forward by Jardine et al. (2006)
 regarding the dependence of X-ray emission on both rotation rate and mass.

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

As some of our targets are faint (V~15) we cannot observe when the moon
 is too close.

Time-Critical Aspects

```
N/A
```

Special Execution Requirements

```
N/A
```

Special Calibration Information

Standard calibrations will be sufficient for our purposes.

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
```

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 15:40:17 2009
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