README web version of /home/usg/OPS/MTS/readme_xml/readme_76013300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program aims at obtaining beryllium and oxygen abundances for a large
sample of
halo and disk stars. The ratio between alfa elements and iron vs. beryllium will
be
used to investigate the formation of the erly Galaxy.
We also observe the stars in the Li region because we check if the
stars are depleted in Li; this is the main reason why we use 2 red
setups: to obtain halfa and Li in one, the oxygen triplet in the other.
Most stars have 2 Obs: each one with a Be observation, while the differ in the red
setups.
A few stars have only one OB: Be UVES archive data for these stars exist, but of
not sufficient
S/N ratio. So they are observed only once.
As a general rule, if possible, we would prefer that for each star
both OBs are executed before moving to another object OB.
No limitations have been set in seeing; in the UV, however, high airmass
implies a very strong decrease of the signal.
Given that the stars are very bright and have hipparcos coordinates, no finding
charts
are associated. We will in the next weeks further check all stars to see if
any potentially doubtful case were present.
Waiver Requests
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 need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:09 2009
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