README web version of /home/usg/OPS/MTS/readme_xml/readme_76502400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We aim at high S/N spectra of the B-type main sequence star HE0437-5439
(B=16.2mag). Due to rotation the lines are somewhat broadened. Therefore non-optimum
resolution is sufficent and a wide slit of 1.4" is acceptable. Therefore we can
accept mediocre seeing conditions up 1.4". The total integration time is split in
9 individual exposures to be executed in
five OBs.
In order to maximise S/N should be observed at low airmass (<=2.0) and good transparancy.
For proper rectification we want to observe a DC-White dwarf, WD1055-072 (B=14.33mag).
We changed the DC with respect to the proposal for better accessibility. Note that
the
star has a HIGH proper motion: p.m.(alpha)=-0.79"/yr; p.m.(delta)=0.08"/yr!
S/N has been estimated with the UVES ETC using a blackbody of the appropriate temperature,
airmass=2.0, seeing=1.4", slit width=1.5", 7 days from New Moon.
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 15:40:11 2009
If you have comments, please contact usd-help@eso.org