README web version of /home/usg/OPS/MTS/readme_xml/readme_79014900

Principal Investigator Email Address

```
jura.borissova@uv.cl
```

Estimated Total Execution Time (hours, including overheads)

```
25:33:06
```

General Description

The goal of the project is to determine the spectral types with MR spectroscopy
 of selected stars in each of 9 photometrically confirmed young clusters close to
 the Galactic center.

Waiver Requests

```
No Waiver Request was submitted
```

Critical Observing Condition Constraints

There are priorities 1 and 2, but they are not critical.

Time-Critical Aspects

```
no
```

Special Execution Requirements

Please note, that always 2 stars shall go into the slit. The slit is centered
 on the one of the targets given in the "User comments" in each OB.
On the finding charts the slit sometimes looks a bit off, but the slit drawing is
 just qualitatively and the targets should always be centered on the slit.
The PA in the acquisition template is approximate and the slit should be rotated
 to fine-tune of both targets.
The OB db2003_106_obj1_2 contains bright object. If it is saturated, please decrease
 the exposure time.
The OB db2003_107_obj1_2 contains 2 bright objects. If it is saturated, please decrease
 the exposure time.
The OB db2003_164_obj1_2 contains 2 bright objects. If it is saturated, please decrease
 the exposure time.
There are relatively large distance between the objects in the OB rcw87_field2_obj21_22
  and rcw87_field1_obj1_2. The nod is 15 arcsec, but please check that the two objects
 are in the slit during the nodding.

Special Calibration Information

Please, observe OV or B0V-B5V telluric standards.
The two OBs with radial velocity standards are prepared. They are very bight stars
 with Ks=6.95 for HD191636 and Ks=7.87 for HD 167785. Please, check for the saturation.

ToO Information

```
No
```

ToO Activators List

```
No
```

Is this a Pre-imaging run ?

```
false
```

Pre-imaging Requirements

```
No
```

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 ?

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 ?

Have you included OBs for any calibrations that you need but which are not part of the Calibration Plan ?

If you are observing Moving Targets, have you attached suitable ephemeris files to your OBs?

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 ?

If you submitted OBs for standard stars, did you use the provided StandardStar templates ?

If you are using a specific offset pattern or position angle, did you check carefully the definition in the manual ?

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 ?

Last creation of page: Tue Oct 6 15:40:18 2009
If you have comments, please contact usd-help@eso.org