README web version of /home/usg/OPS/MTS/readme_xml/readme_82072600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We look for small (20%) abundance differences in differently evolved stars
(main sequence, turn-off, subgiant and red-gaint stars) of the solar-metallicity
open cluster M67. Such abundance differences would indicate that atomic diffusion
is at work in these stars which could help resolve problems in matching the observed
colour-magnitude diagram with isochrone computed using the latest (low) solar abundance
mixture (see VandenBerg et al. 2007, ApJ 666, L105).
Data homogeneity is of critical importance to this project.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
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 ?
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 15:40:27 2009
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