We present preexplosion optical and infrared (IR) imaging at the site of the type II supernova
(SN II) 2023ixf in Messier 101 at 6.9 Mpc. We astrometrically registered a ground-based …

Pair-instability supernovae are theorized supernovae that have not yet been observationally
confirmed. They are predicted to exist in low-metallicity environments. Because overall …

We measure the molecular gas environment near recent (< 100 yr old) supernovae (SNe)
using∼ 1''or≤ 150 pc resolution CO (2–1) maps from the PHANGS–Atacama Large …

The Gamow Explorer will use Gamma Ray Bursts (GRBs) to: 1) probe the high redshift
universe (z< 6) when the first stars were born, galaxies formed and Hydrogen was reionized; …

Core-collapse supernovae (CCSNe) are widely accepted to be caused by the explosive
death of massive stars with initial masses≳ 8 M⊙. There is, however, a comparatively poor …

We present a statistical analysis of the local,≈ 50–100 pc scale, Hα emission at the
locations of recent (≤ 125 yr) supernovae (SNe) in nearby star-forming galaxies. Our …

We reexamined the classification of the optical transient ASASSN-18ap, which was initially
identified as a supernova (SN) upon its discovery. Based on newly emerged phenomena …

In this work we estimate the explosion and progenitor properties of six Type II supernovae
(SNe) at 0.675<= z<= 3.61 discovered by the JWST Advanced Deep Extragalactic Survey …

Neutrino telescopes such as IceCube monitor for low-energy neutrinos O (10 MeV)
produced in nuclear processes during core-collapse in supernovae. The detection horizon …

Aims. We present a detailed analysis of SN 2020qmp, a nearby Type IIP core-collapse
supernova (CCSN) that was discovered by the Palomar Gattini-IR survey in the galaxy …