README web version of /home/usg/OPS/MTS/readme_xml/readme_76081000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a low resolution spectroscopic run on HB stars in the Omega Centauri
field.
Spectroscopy is performed by FORS2 (grism=600B+22, slit=0.51'') on 233 stars
with B-V < 0.50.
The goal is to provide new observational inputs in the attempt to understand
the nature and the formation history of Omega Centauri by investigating the
Helium content, temperatures and gravities of its HB stars with Teff >= 10000
K.
Waiver Requests
In order to maximize the number of useful targets, we realized
that the best solution is obtained using 12 (twelve) MXU masks
(still staying within the assigned 17 observing hours, including
overheads): this in order to avoid the too crowded internal region
of the cluster (Omega Centauri).
Because the program requests the observation of the largest number
of targets (for statistical reasons) we request to be allowed to
exceed the limit of the ten masks.
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
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 have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS2 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:11 2009
If you have comments, please contact usd-help@eso.org