README web version of /home/usg/OPS/MTS/readme_xml/readme_82064602
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This observation aims at studying the optical counterpart of a triple
X-ray source P8 in the galaxy NGC 7793. The X-ray source is well aligned with a
supernova remnant candidate S26 and the central X-ray source appears coincident
with a blue ~23 mag star.
We propose here to carry spectroscopic observations to study the bubble and the
stellar counterpart.
The 4 spectroscopic observations should be carried out randomly. The standard configuration
will be LSS Grism 300V+10 with no filter and slit width of 1.0\", slit orientation
along the triple X-ray source (rotator = +32.1deg).
One extra spectrum will use LSS Grism 600V+94 with the GG375+30 filter and slit
width of 0.7" and slit orientation as above.
The finding chart is showing the target for which there is the need to use a blind
offset.
As we got a special authorization to change the moon constraint, we have now 1.5
guaranteed hour that we would like to use for one spectrum with grism 300V and one
spectrum with grism 600V (OBs 0 and 3). The two others OB correspond to the 1.5
hour on hold.
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 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 15:40:27 2009
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