README web version of /home/usg/OPS/MTS/readme_xml/readme_75035200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
These observation make up a continuing survey of magnetic fields in hot
subdwarfs. There are 22 targets, ranging from hydrogen-rich sdB and sdO to helium-rich
sdO stars. Each target has one science OB and two calibration OBs (to be done during
the day). Each calibration OB is identical. The science OBs contain typically three
exposures at two different retarder waveplate settings (i.e. six total), allowing
a S/N of 1000 or greater to be achieved. The circular polarisation of H and He lines
will be measured, the magnetic field strength will be determined and compared with
other stellar parameters.
Waiver Requests
One waiver request was submitted (075.D-0352A.01.WAV), and was approved,
to allow the use of the low gain mode of the CCD amplifier for these observations.
This will allow fewer exposures on each target, meaning more time spent integrating.
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
Since the observations are being made with a non-standard setting, extra
calibration frames need to be taken. There are two calibration OBs for each target,
one for flat fields and biases (subdwarf Cal Bias+Flat-*) and one for arc spectra
(subdwarf Cal Arc-*). At the very least, the arc spectra should be taken during
the day after each run, but it is preferable that both OBs are carried out for each
target.
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 have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS1 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:07 2009
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