README web version of /home/usg/OPS/MTS/readme_xml/readme_60943500
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We propose to obtain X-Shooter spectra of one quasar within the
Deep-02h VVDS Field in order to cross-correlate their Ly-$\alpha$ 1215
\AA, CIV 1548-1550 \AA\ and MgII 2796-2803 \AA\ absorbers with the
7972 foreground galaxies with secure spectroscopic redshifts. The
CFHTLS-D1-02h equatorial field has been extensively observed by the
magnitude-selected VVDS Deep spectroscopic VIMOS survey yielding
reliable spectroscopic identifications for several thousands objects
between z = 0 and z = 5. It is a pure I-band limited dataset for which
the 2D spectra have been observed and redshifts accurately measured
with spectral features such as the Lyman break, the Ly-alpha emission,
the FUV absorption lines, etc. Spectroscopic redshifts are reliable at
a Delta(z)=0.005 level. The selection function is well-controlled
through the whole redshift baseline up to z~5. Here, we propose to
make use of the UV to IR coverage of X-Shooter to look for absorbers
in the spectra of some of the quasar in the field.
Target:
VVDS020268754 36.5401181 -4.4105422
V mag=20.60 z_em=2.7187
slit mode
PA=0
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