SVOM's Visible Telescope reaches 0.03 arcsec astrometric precision for bright stars and 0.02 mag photometric stability after recovering from contamination via bake-out.
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The GWAC array monitors 3600 square degrees of sky with 40 cameras for prompt optical emission from gamma-ray bursts, achieving 16th magnitude sensitivity in 10-second exposures.
citing papers explorer
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SVOM/VT: Preliminary Calibration Analysis
SVOM's Visible Telescope reaches 0.03 arcsec astrometric precision for bright stars and 0.02 mag photometric stability after recovering from contamination via bake-out.
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Overview of Ground-based Wide-Angle Cameras array
The GWAC array monitors 3600 square degrees of sky with 40 cameras for prompt optical emission from gamma-ray bursts, achieving 16th magnitude sensitivity in 10-second exposures.