1550nm fiber optic components, vis-2000nm free space optics, super-stable fiber optic laser, diode lasers for 800-1630 nm, fiber optic amplifier (5W), microwave synthesizer 0.5 –20 GHz, microwave amplifiers , sub-mm and terahertz detectors (for room temperature (Golay-cell) and cryogenic, cold head), microwave spectrometer, high resolution Olympus microscope (limited by diffraction), 2 35 cm Dobsonian optical telescopes. of diameters, ROACH platform (to perform correlator), clean room air filters, equipment borrowed from ALMA.