2 citations · 5 across the 9 of their papers we have counts for
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A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13
David A. Coulter, Conor Larison, Justin D. R. Pierel +88
Observing supernovae (SNe) in the early Universe (z > 3) provides a window into how both galaxies and individual stars have evolved over cosmic time, yet a detailed study of high-r…
Expanding the High-z Supernova Frontier: "Wide-Area" JWST Discoveries from the First Two Years of COSMOS-Web
Ori D. Fox, Armin Rest, Justin D. R. Pierel +48
Transient astronomy in the early Universe (z > 2) remains largely unexplored, lying beyond the rest-frame optical spectroscopic reach of most current observatories. Yet this regime…
The rates and host galaxies of pair-instability supernovae through cosmic time: Predictions from BPASS and IllustrisTNG
Max M. Briel, Benjamin Metha, Jan J. Eldridge +2
Pair-instability supernovae (PISNe) have long been predicted to be the final fates of near-zero-metallicity very massive stars (, $\mathrm{M}_\mathrm{ZAMS} \gtrsim 1…
Superluminous supernovae
Takashi J. Moriya
Superluminous supernovae (SLSNe) are a population of supernovae (SNe) whose peak luminosities are much larger than those of canonical SNe. Although SLSNe were simply defined by the…