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A candidate microlensing event toward the Galactic bulge

Contribution grade

Astrophysics · Source-reported experimental result or reusable measurement method

Reference score90,000Provisional editorial estimate of this exact contribution; its grade is assessed separately.

What changed

The OGLE team reported a candidate microlensing event toward the Galactic bulge after surveying approximately 650,000 stars. The selected star brightened and returned to its previous level; a single-lens model fit its light curve with an estimated Einstein-radius crossing time of 23.8 ± 0.9 days. This was a separate direction and event from contemporaneous Large Magellanic Cloud searches.

Scientific scope

The OGLE team reported a candidate microlensing event toward the Galactic bulge after surveying approximately 650,000 stars. The selected star brightened and returned to its previous level; a single-lens model fit its light curve with an estimated Einstein-radius crossing time of 23.8 ± 0.9 days. This was a separate direction and event from contemporaneous Large Magellanic Cloud searches. The rising light curve was poorly sampled and the observers could not test achromaticity during the event because V-band coverage was sparse. The paper treats the event as a candidate and cannot exclude an unusual variable star. Its likely approximately 0.3-solar-mass disk-lens estimate is conditional on a population and geometry model, not a direct mass or lens-type measurement. The distinct MACHO and EROS event teams retain their own credits; do not equate their timescale definitions or samples.

Evidence

The linked original works support the scoped statement and contribution attribution. WRS has not independently replayed experiments or reconstructed a full mathematical proof. The rising light curve was poorly sampled and the observers could not test achromaticity during the event because V-band coverage was sparse. The paper treats the event as a candidate and cannot exclude an unusual variable star. Its likely approximately 0.3-solar-mass disk-lens estimate is conditional on a population and geometry model, not a direct mass or lens-type measurement. The distinct MACHO and EROS event teams retain their own credits; do not equate their timescale definitions or samples.

Contributors

Provisional WRS assessment, edition 2026-10-28.1. Independent expert calibration is pending. This grade does not certify correctness or assign ownership.

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