README web version of /home/usg/OPS/MTS/readme_xml/readme_75080700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Beryllium and Nitrogen in NGC~6752: a critical test for the cluster formation
The program aims at measuring Beryllium abundances in 2 Torn Off stars of the globuar
cluster NGC6752. Easch star is observed 10 times with the same OB for 1.5 hours.
The magnitude of the stars is V~17.2 and we are attempting a measurement about 1
magnitude fainter than ever obtained in the past. we are pushing at the limits.
Being in the extreme UV, it is important not to exceed the airmass constraints and
to observe the stars as much as possible close to meridian. Finding charts are from
UVES slit viewer previous observations. In case the programme cannot be concluded,
n4428 should be observed and finished first (set in the priorities).
If I could access some of the reduced data prior program completion, it could be
very very useful.
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 15:40:08 2009
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