README web version of /home/usg/OPS/MTS/readme_xml/readme_79007300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We intend to analyse a sample of O stars of NGC 346, the largest HII region
in the SMC. The analysis will be based on high-resolution spectra and NLTE models,
and will account for NLTE metal line blanketing, spherical extension, and stellar
winds. We will derive for each star the basic stellar parameters, apparent rotational
velocities, surface chemical composition and wind properties. This analysis will
allow us to obtain a map of CNO abundances across the parameter range of O stars,
probing the efficiency of rotationally-induced mixing. To achieve our science goals,
near-UV spectra are critical and we need a S/N > 60 in this wavelength range
to properly derive oxygen abundances.
Finding charts have been obtained from ALADIN. We could not reach a better quality
for the field size of 1x1 arcminutes, as the targets are quite faint and the fields
crowded. The targets are always at the center of the FC and indicated by a (pink)
cross and a down arrow.
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 15:40:17 2009
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