Sub-arcsecond FIR observatory: a science imperative. In the L2/L3 era, the FIR domain will present a severe gap in resolution and sensitivity between ALMA and JWST/E-ELT. The band maps on key tracers: dust continuum peak, and features tracing composition and formation.
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TALC 20m annular telescope
FIRIT 36m direct imaging interferometer
ESPRIT ~50m free-flying heterodyne interferometer
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