The NUTTelA-TAO system consists of three parts:  The telescope, the burst simultaneous three-channel instrument (BSTI), and the automated fast roof system. The BSTI is really three cameras in one, each measuring the same part of the sky in different colors (using Sloan i’, r’, g’ filters) at precisely the same time, sometimes called “hyperspectral imaging”.  This allows us to measure the shape of the emission spectrum at three different wavelengths, even for our fast transients. Conventional astronomical cameras have one camera and a filter wheel that is moved between images; these cannot be used to measure rapidly-changing transient targets as they change too much between exposures, while the filter wheel is moving. The BSTI machining and optical assembly is 100% made in Kazakhstan by ECL scientists and engineers from the NU and ECL machine shops.