README web version of /home/usg/OPS/MTS/readme_xml/readme_81046600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program targets two white dwarfs which have gaseous, volatile-element
depleted debris discs. The debris discs are unveiled double-peaked emission lines
in the CaII 860nm triplet, and by FeII 517nm. Various metal lines in the photosphere
of the white dwarf show that the star is accreting from the debris disc. The aim
of these observations is to provide high-resolution data of the emission lines of
the discs and of the absorption lines from the white dwarf.
Having received a first set of UVES data from a previous observing programme on
one of the targets, SDSS1228+1040, we have slightly modified the strategy with respect
to the Phase I proposal: we have dropped a third, fainter target for which the data
would have been marginal, and decided to spend more time on the 517nm Iron lines.
Please try to carry out the OB SDSS1228_437+760 a bit later in Period 81, preferably
from mid-June onwards, as this will help in establishing the level of variability
in the CaII emission lines (by comparison with our 2007 UVES data).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Please try to carry out the OB SDSS1228_437+760 a bit later in Period
81, preferably from mid-June onwards, as this will help in establishing the level
of variability in the CaII emission lines (by comparison with our 2007 UVES data).
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 15:40:24 2009
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