README web version of /home/usg/OPS/MTS/readme_xml/readme_83013001
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
In this observing run the B components of two bright double star systems
shall be observed. Weak absorption lines of the material of the mass losing main
component shall be detected.
There are 4 OBs, 2 for each system, to get spectra with both blue cameras of UVES.
Acquisition takes place on the weaker B component in each case. The slit is rotated
to the position angle of the binaries to eventually get spatial resolved spectra
of the circumstellar matter. For alpha Herculis both components are located in the
slit, while for BO Carinae the B component is located at one end of the slit to
put the slit as near as possible to the main component.
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 specified the S/N ratio at given wavelength in the User Comments
field of each OB?
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 15:40:29 2009
If you have comments, please contact usd-help@eso.org