README web version of /home/usg/OPS/MTS/readme_xml/readme_79013101
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This run aims at obtaining high resolution (R~50000) and high S/N (~100)
spectra of 3 dwarfs in the stellar cluster NGC 2447. This program is
a complement to the run A, where a series of giant stars of 13 clusters
are observed.
These dwarfs were chosen based on observations taken in a separate
program to search for planets around stars of this cluster.
These stars are not spectroscopic binaries, and they rotate slowly.
These observations will be used to derive the chemical abundances in
the cluster.
Observations are to be done with UVES using the red 580 mode,
and a slit of 0.9'' (R~50000). Although the fields are relatively crowded,
the introduction of a slit angle was not judged necessary in any of the
cases.
Once the three stars of NGC2447 are observed, please give priority
to observe the three giants of the same cluster listed in Run A of this
program (if observations of these were not done yet).
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 15:40:18 2009
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