README web version of /home/usg/OPS/MTS/readme_xml/readme_60942900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The goal of this program is to study mass-accretion rates in Herbig Ae
stars with detected magnetic fields. No finding chart was submitted, as the approved
targets are bright and do not have nearby bright companions.
The visual magnitudes of targets are:
V=7.3 for HD176386
V=7.8 for HD190073
V=10.7 for for PDS2
For the observation of the telluric standard star, we would like to get a solar
type star. At large zenith distances the slit should be placed at the parallactic
angle.
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 ?
Last creation of page: Tue Oct 6 15:40:06 2009
If you have comments, please contact usd-help@eso.org