Overview
- The study appearing in The Astrophysical Journal argues that a close interaction or merger between a massive, helium-rich star and a black hole companion best explains SN 2023zkd’s unusual explosion.
- The Light curve Anomaly Identification and Similarity Search (LAISS) AI tool flagged the transient months before its peak, allowing rapid, multi-instrument observations of its rise and fall.
- Archived data show the progenitor brightened gradually over more than four years prior to detonation, an extremely rare pre-explosion signal for supernovae.
- Photometric and spectroscopic analysis reveals a double-peaked light curve produced by the blast’s sequential collisions with low-density circumstellar gas and a denser, disk-like cloud.
- Researchers say this event provides some of the strongest observational evidence that compact companions can trigger or reshape massive-star explosions and highlight the need for AI-driven triage ahead of the Rubin Observatory era.