README web version of /home/usg/OPS/MTS/readme_xml/readme_80028800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Constraining the time variation of dimensionless physical constants is
crucial for our understanding of physics. We propose to use the unique capabilities
of UVES to strengthen the constraint on the variation of the electron-to-proton
mass ratio
(mu=me/mp) by measuring precisely the wavelength of molecular hydrogen transitions
in high-redshift damped Lyman-$\alpha$ systems. We have discovered two new H2 bearing
DLAs presenting close to ideal characteristics for such measurement:
(i) large redshift, z=2.402 and 2.658,
(ii) simple absorption profile, a single Gaussian and
(iii) intermediate H$_2$ column densities, log N(H2)=17.30 and 18.41, with absorptions
from several rotational levels.
Together with the two systems from the literature (Ivanchik et al. 2005), these
new observations will yield about 150 aborption lines. About thirty will be in common
to at least two quasars. This will definitely solve the issue of a variation of
mu at a level achievable with present-day instrumentation.
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 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 15:40:21 2009
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