General |
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SofI is the infrared spectrograph
and imaging camera on the NTT. Its largest field of view is
4.92 arcmin, and it covers the 0.9-2.5 micron wavelength
range with spectral resolution from 600 to 2200.
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Built by:
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ESO |
P.I.: |
A. Moorwood |
Instrument Scientists: |
Julia Scharwächter and
Alessandro Ederoclite |
System Engineer: |
Javier Valenzuela |
Instrument Friend: |
Manuel Pizarro |
Location: |
NTT, Nasmyth A |
Publication reference: |
Moorwood, A., Cuby, J.G., Lidman, C. 1998, The Messenger 91, 9 |
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Previous Intrument Scientists
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Valentin D. Ivanov (until June 2007)
Cédric Foellmi (2nd IS, until Apr 2006)
Malvina Billeres (until Apr 2004),
Leonoardo Vanzi (until Sep 2002),
Chris Lidman (Golden Age),
Jean-Grabriel Cuby (Good Old Times) |
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News |
SofI Status (for previous updates click
here):
- There was a successful SofI intervention to fix a vacuum leak in mid-April. The instrument is back in good condition.
(Apr 2007)
- The small field and large field + focal elongator modes are decommissioned because of a persistent collimator problem;
it is not planned to recommission them for now. (Feb 2007)
- New imaging templates AutoJitterRot and JitterRot are available starting P80; they allow to rotate the instrument between
the exposures. (Feb 2007)
- FastPhotometry mode is available starting P80, only in Visitor Mode; it allows to carry out imaging
observations with high time resolution, as high as 10-20 milisec, windowing the detector array down to 20-30 sq. pixels;
contact the SofI instrument scientist for details. (Feb 2007)
Updates (for previous updates click
here):
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Please mail to ls-sofi for comments, suggestions and to report errors and inaccurate statements in the web pages and manuals.
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