DARTS

Currently, large-scale celestial surveys such as the Vera C. Rubin Observatory have increased the demand for spectrographs to classify celestial objects and determine their properties. In response to this need, NARIT, in collaboration with Lick Observatory in the United States, has developed the Dual-beam Automatic Rapid Transient Spectrograph (DARTS) for installation on the 2.4-meter telescope at Lick Observatory in California, USA.

Dual-beam Automatic Rapid Transient Spectrograph is designed for automated observations, making it suitable for tracking transient objects such as variable stars, active galaxies, or supernovae. It features a resolution of 1,000 and utilizes a K-mirror system for light guidance. This collaboration with Lick Observatory enhances NARIT's capability in developing optical instruments in partnership with leading international observatories.