README web version of /home/usg/OPS/MTS/readme_xml/readme_75051100
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
1) We have basically one target of interest which is V4332 Sgr. We wish
to take spectra of
it in 2 spectral regions using UVES. The first UVES spectrum covers 476-678nm (the
present README file pertains to this spectrum). The second spectrum covers 676-1052nm
(which simultaneously gives a blue spectrum at central w.l. of 437 nm)
2) We are a little concerned at not including standard calibrations for the spectra
at point 1 as separate OBs. But we understand that a flatfied, bias and spectral
calibration data are provided by the observatory and need not be included as OBs.
This is what is stated in Section 9.2 of the UVES Templates Reference Guide (Doc
VLT-MAN-ESO-13200-1567). In case our understanding is wrong, such calibration data
"MUST" be taken and the time for it can be adjusted by reducing the target OBs accordingly
3)Since both the spectra mentionted in point 1 above will have telluric lines which
we wish to remove, we are taking corresponding spectra of the standard star LTT
7987. This object has similar RA and Dec values as the target and therefore similar
airmass. This is a hot white dwarf which is expected to have a featureless continuum
except for telluric features.
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 15:40:07 2009
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