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ZEUS-2, the second generation (z)Redshift and Early Universe Spectrometer,like its predecessor is a moderate resolution (R~1000) long-slit, echellegrating spectrometer optimized for the detection of faint, broad lines fromdistant galaxies. It is designed for studying star-formation across cosmictime. ZEUS-2 employs three TES bolometer arrays (555 pixels total) to deliversimultaneous, multi-beam spectra in up to 4 submillimeter windows. The NISTBoulder-built arrays operate at ~100mK and are readout via SQUID multiplexersand the Multi-Channel Electronics from the University of British Columbia. Theinstrument is cooled via a pulse-tube cooler and two-stage ADR. Various filterconfigurations give ZEUS-2 access to 7 different telluric windows from 200 to850 micron enabling the simultaneous mapping of lines from extended sources orthe simultaneous detection of the 158 micron [CII] line and the [NII] 122 or205 micron lines from z = 1-2 galaxies. ZEUS-2 is designed for use on the CSO,APEX and possibly JCMT.

ZEUS-2: a second generation submillimeter grating spectrometer for exploring distant galaxies