Status: Private Instrument; (T. Soifer, K Matthews)
5.4" x 9.6", rotatable to any position angle
0.67", or 4 pixels
0.167" per pixel with D80
0.125" per pixel with D78
D80;256 x 256 HgCdTe, 1-2.5 micron
D78;256 x 256 InSb 1-5 micron, (does not cover entire PIFS field of view)
f/70 tip/tilt corrected beam
f/70 beam matched to focal plane of imaging camera.
High Resolution R = 1300
Low Resolution R = 550
5,000 km/sec in High Resolution mode
12,000 km/sec in Low Resolution mode
10-20 km/sec on high signal to noise narrow lines.
Less than one pixel at the focal plane for large telescope motion.
PIFS alone 58%. Total system including atmosphere, telescope, and camera is about 22%.
Sensitivity: 5x10-16 erg s-1 cm-2 at the 3-sigma level in 30 minutes of integration for a spatially and spectrally unresolved line emission source in 1-arcsecond seeing.
In the best of seeing conditions (0.5 arcsec), predicted sensitivity is a K=18 (0.04 mJy) continuum source at 5-sigma in one hour of integration.
In excess of three days in lab.
Full field imaging capability for target acquisition.
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Contact:
Jeff Hickey |
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