Wide-field-of-view infrared cameras, operating on the new generation of lar
ge telescopes, offer unprecedented gains in the detection of faint sources
and in observing efficiency for both direct imaging and spectroscopy. With
a 1024 x 1024 pixel, 1-2.5 mum detector, the PISCES camera provides 8.'5 an
d 3.'16 fields at the 2.3 m Bok telescope and 6.5 m Multiple Mirror Telesco
pe, respectively. Its refractive optics utilize all spherical surfaces and
standard glasses. A cold pupil stop suppresses the thermal background produ
ced by the emissive surfaces normally present in Cassegrain optical configu
rations. The optical design is directly extendable to wider fields with lar
ger detector formats. Future upgrades include low-resolution (R = 200-500)
multiobject spectroscopy.