Type IIn supernovae are luminous core-collapse explosions of massive stars that, unlike other types, are very bright in the ultraviolet and have strong, long-lived emission lines that should enable detection at redshift z ≈ 2. Here, three spectroscopically confirmed type IIn supernovae are reported at redshifts z = 0.808, 2.013 and 2.357, detected in archival data.
- Jeff Cooke
- Mark Sullivan
- Erik Tollerud