DREAMS DR1 provides ~59 million bulge star light curves at minute cadence to z~22, with a pilot search yielding one microlensing event, two flares, and 24 new short variables.
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N6946-BH1's remnant is roughly 10 times fainter than its progenitor while stellar merger remnants are 10-100 times brighter, and asymmetric dust cannot explain the difference.
Non-detection of TDE in IC230724A; LSST could constrain TDE fraction of neutrino background to ≲60% or ≳30% with 10 events.
citing papers explorer
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A Minute-Cadence Deep Bulge Survey: First Data Release of DREAMS
DREAMS DR1 provides ~59 million bulge star light curves at minute cadence to z~22, with a pilot search yielding one microlensing event, two flares, and 24 new short variables.
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The neighboring stars of N6946-BH1 and the observational characteristics of failed supernovae
N6946-BH1's remnant is roughly 10 times fainter than its progenitor while stellar merger remnants are 10-100 times brighter, and asymmetric dust cannot explain the difference.
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Deep Optical Follow-up Observations to IceCube Cosmic Neutrinos: a case for IC230724A with Subaru/HSC and prospects with Rubin/LSST
Non-detection of TDE in IC230724A; LSST could constrain TDE fraction of neutrino background to ≲60% or ≳30% with 10 events.