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Long Gamma-Ray Bursts Doubled Their Supernova-Less Candidate List

Two decades of Swift data produced a rate of 0.5 ± 0.2 events per cubic gigaparsec per year before beaming correction.

Published Updated Story ID: mp-2026-09-19-015
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Summary

Two decades of Swift data produced a rate of 0.5 ± 0.2 events per cubic gigaparsec per year before beaming correction.

A search below redshift 0.35 more than doubled the candidate set with robust supernova limits and distance scales. The small, heterogeneous sample spans star-forming, dusty and quiescent hosts; plausible beaming corrections remain compatible with several compact-merger channels but do not establish one origin.

Why it matters

Two decades of Swift data produced a rate of 0.5 ± 0.2 events per cubic gigaparsec per year before beaming correction.

Limits and context

  • The small, heterogeneous sample spans star-forming, dusty and quiescent hosts; plausible beaming corrections remain compatible with several compact-merger channels but do not establish one origin.

Key claims

  1. Two decades of Swift data produced a rate of 0.5 ± 0.2 events per cubic gigaparsec per year before beaming correction.

    Qualification: The small, heterogeneous sample spans star-forming, dusty and quiescent hosts; plausible beaming corrections remain compatible with several compact-merger channels but do not establish one origin.

    Evidence: source-2026-09-19-017

Sources

  1. arXiv preprint 2609.20787arXiv · primary research

Corrections

No corrections have been recorded for this story.