README web version of /home/usg/OPS/MTS/readme_xml/readme_75063700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We propose to observe at high spectral resolution a sample of Herbig stars
for which we have already measured the amount of circumstellar molecular hydrogen
from FUSE data. The analysis of interstellar and/or circumstellar lines at optical
wavelengths, especially CH and CH+ lines, combined to our H2 data, will allow us
to explain the chemical mechanisms of formation/destruction and excitation of the
different molecules in the circumstellar environment of HAeBes.
We absolutely need the maximum spectral resolution (~80,000, slit width=0.4) to
separate the different gaseous components along the line of sight. High S/N ratio
(S/N>150) is required to detect the very weak CS lines one would expect to observe
in the CS environment of our target stars. Indeed, although CH absorption lines
are generally broad, lines of CH+ are very weaker and are the most important lines
in our study to constrain the excitation conditions of the CS gas.
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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