The First Light APEX Submillimeter Heterodyne (FLASH) instrument was installed at the Nasmyth–A Atacama Pathfinder Experiment (APEX) telescope on the Chajnantor plateau in Chile’s Atacama region in 2004. The development of FLASH was a collaboration between SRON and the University of Cologne.
FLASH was a dual-frequency receiver that operated simultaneously on orthogonal polarisations in the 0.65 mm (460 GHz) and 0.87 mm (345 GHz) atmospheric windows. In its first incarnation FLASH was equipped with a 0.37 mm (810 GHz) and a 0.65 mm (460 GHz) channel. It had a wide tuning range between 0.34 and 0.38 mm (780 and 880 GHz) and between 0.60 and 0.71 mm (420–500 GHz) and intermediate frequency bandwidths of 2 and 4 GHz, respectively. It was the high-frequency heterodyne workhorse during the commissioning of the APEX in its first years of operation. After the successful installation of the CHAMP+ array, also covering the 0.37 mm (810 GHz) atmospheric window, the high-frequency channel was replaced with a state-of-the-art sideband separating 0.87 mm (345 GHz) detector.
FLASH instrument was decommissioned in 2012 and replaced with FLASH+.
FLASH on APEX technical specifications
This table lists the global capabilities of the instrument. The authoritative technical specifications as offered for astronomical observations are available from the Science Operations page.