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A predicted gravitationally lensed supernova image reappears

Contribution grade

Observational astrophysics · Source-reported experimental result or reusable measurement method

Reference score155,000Provisional editorial estimate of this exact contribution; its grade is assessed separately.

What changed

After four images of supernova Refsdal were observed in 2014 behind galaxy cluster MACS J1149.5+2223, five modeling teams used existing imaging and spectroscopy to construct seven lens models and predicted an additional image. Hubble observations on 11 December 2015 revealed a new source at the predicted location, interpreted as that fifth image. Its early brightness and timing allowed a blind comparison with prior lens-model predictions. A later blinded analysis of the extended light curves reported an SX–S1 delay of 376.0 days with a 16th–84th percentile interval of approximately −5.5 to +5.6 days, using a weighted combination of four fitting methods.

Scientific scope

After four images of supernova Refsdal were observed in 2014 behind galaxy cluster MACS J1149.5+2223, five modeling teams used existing imaging and spectroscopy to construct seven lens models and predicted an additional image. Hubble observations on 11 December 2015 revealed a new source at the predicted location, interpreted as that fifth image. Its early brightness and timing allowed a blind comparison with prior lens-model predictions. A later blinded analysis of the extended light curves reported an SX–S1 delay of 376.0 days with a 16th–84th percentile interval of approximately −5.5 to +5.6 days, using a weighted combination of four fitting methods. This is a later image of the same explosion, not a new explosion. The seven forecasts share observational inputs and are not seven independent confirmations. In the October 2015 forecast most models predicted the peak in the first quarter of 2016; the December detection is an appearance, not the date of the peak. The early light curve constrains time delay and magnification jointly; full light-curve fitting and systematic errors including mass-sheet degeneracy and line-of-sight structure remained open. The pre-observation forecast and subsequent observation have distinct source-specific bylines. The later delay and its uncertainty depend on light-curve models, simulation-calibrated method weights and microlensing assumptions; a companion Hubble-constant inference is a separate analysis. In the v1 corner-plot figure, some short-delay labels differ from the primary delay table and figure; those values need reconciliation and are not exported.

Evidence

The linked original works support the scoped statement and contribution attribution. WRS has not independently replayed experiments or reconstructed a full mathematical proof. This is a later image of the same explosion, not a new explosion. The seven forecasts share observational inputs and are not seven independent confirmations. In the October 2015 forecast most models predicted the peak in the first quarter of 2016; the December detection is an appearance, not the date of the peak. The early light curve constrains time delay and magnification jointly; full light-curve fitting and systematic errors including mass-sheet degeneracy and line-of-sight structure remained open. The pre-observation forecast and subsequent observation have distinct source-specific bylines. The later delay and its uncertainty depend on light-curve models, simulation-calibrated method weights and microlensing assumptions; a companion Hubble-constant inference is a separate analysis. In the v1 corner-plot figure, some short-delay labels differ from the primary delay table and figure; those values need reconciliation and are not exported.

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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