README web version of /home/usg/OPS/MTS/readme_xml/readme_60942800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Simple broad-band spectroscopy of well-known Galactic black hole candidate
GX 339-4. The aim is to detect a spectral break (slope change) expected in the near-IR
due to the transition from a jet to an accretion disc-dominated spectrum.
Finding chart 1 : 60.A-9428_001.JPG : Large field-of-view image
Finding chart 2 : 60.A-9428_002.JPG : Zoom in, also indicating large source variability
and suggested slit angle.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Simple observation of bright(ish) point source.
* Just watch out for a nearby star almost exactly 5 arcsec south of target.
* And note that the source is highly variable, with typical V~16-18, but minimum
and maximum ranges are over V~15-20; I attach two several finding charts showing
different source states to make acquisition easier.
* I have adjusted exposure Texp, DIT and NINT so that the source does not saturate
even if it happens to be rather bright (V~16). But please feel free to choose a
different setup for better optimization.
* Slit position angle chosen to avoid star 5" south, but angle not critical. Same
for throw value.
Special Calibration Information
None. We simply want accurate cross-calibration between the arms in order
to model the entire continuum. This can be achieved with standard CCD, ARC, TELLURIC
and SPECPHOT calibrations. Any hot telluric star will do.
ToO Information
ToO Activators List
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
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 ?
Last creation of page: Tue Oct 6 15:40:06 2009
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