README web version of /home/usg/OPS/MTS/readme_xml/readme_82061700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The Galactic high-velocity clouds (HVCs) are massive clouds of neutral
hydrogen
gas outside the Milky Way disk, tracing (a) low-metallicity material left over
from the formation of the Milky Way, (b) the Magellanic Stream, a tidal tail
pulled out of the SMC by the Milky Way, and (c) a ``Galactic Fountain'' - the
cycling of gas between the Disk and the Halo. Knowing their distances and
metallicities allows us to estimate the rate of circulation of gas between the
Disk and the Halo, as well as the rate of infall of low-metallicity material.
For the current proposal we have selected three HVCs with known
metallicity, whose distance we intend to determine. The proposed target
list includes a total of 27 stars with known distances toward the three HVCs.
We will use the spectra of these stars to search for interstellar CaII absorption
in the HVCs and to constrain in this way the distances of the clouds. This will
allow
us to place these HVCs in the circumgalactic environment of the Galaxy. The
data will provide crucial new information about the role of the HVCs
for the ongoing formation and evolution of the Milky Way.
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 15:40:27 2009
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