Shortly after the data release, Rubin Observatory played a key role in observing SN 2026gzf, a rare broad-lined Type Ic supernova first detected as the X-ray flash EP260321a by China's Einstein Probe on March 21, 2026, from a galaxy about 500 million light-years away .
Rubin — alongside the Dark Energy Camera, the Mayall 4-meter telescope with DESI, and others — rapidly turned to monitor the event within hours . The observations captured the shock breakout: the moment the blast wave from the stellar explosion burst through the star's surface, releasing the first light of the supernova
. This is described as only the second time in ~20 years that astronomers have captured such an early shock breakout from a massive star's death
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The coordinated global campaign, led by a Carnegie Mellon University team, revealed that SN 2026gzf is among the faintest shock breakouts ever associated with a broad-lined Type Ic supernova, with thermal X-ray emission peaking at 2.2×10⁴⁴ erg/s .
The Rubin Observatory formally began the Legacy Survey of Space and Time (LSST) in late June 2026 — a planned 10-year survey of the Southern Hemisphere sky .
The LSST uses the 3.2-gigapixel camera mounted on the Simonyi Survey Telescope atop Cerro Pachón in Chile to image the entire visible sky every few nights . Over the decade, it will produce an ultra-wide, ultra-high-definition time-lapse movie of the universe, generating the most comprehensive cinematic record ever created
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Some 2,800 scientists from around the world are involved, studying dark energy, dark matter, the structure of the Milky Way, the Solar System (including near-Earth objects), and transient phenomena like supernovae . The survey is designed to capture hundreds of images per night and had already demonstrated its rapid alert capability by issuing 800,000 transient alerts in a single night during commissioning
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