Applications

X-Ray, UV and VUV Spectroscopy

The presence of UV, VUV and X-ray phenomena across the galaxy provides numerous opportunities for observation and research. Photonis has provided a wide range of products to mission experiments that support X-Ray, VUV and UV spectroscopy. These instruments are used to survey and map atmospheric skies, and to identify black holes, neutron stars, binary star systems or other objects emitting these rays. They have been installed on ground-based telescopes or launched as independent research missions.

Some notable missions that Photonis has been a part include:
CHANDRA, CHIPS, FUSE, Hubble COS, ROSETTA, EUVE, ULYSSES, HUT, SAOGBO