We assemble a large set of 2–10 GHz radio flux density measurements and upper limits of
294 different supernovae (SNe), from the literature and our own and archival data. Only 31 …

Modelling the red–blue asymmetries seen in the broad emission lines of core-collapse
supernovae (CCSNe) is a powerful technique to quantify total dust mass formed in the ejecta …

The spectacular outbursts of energy associated with supernovae (SNe) have long motivated
research into their potentially hazardous effects on Earth and analogous environments …

Type IIP supernovae (SNe) are expected to arise from red supergiant stars (RSGs). These
stars have observed mass-loss rates that span more than two orders of magnitude, from less …

We present a systematic study of mid-infrared emission from 141 nearby supernovae (SNe)
observed with Spitzer/IRAC as part of the ongoing SPIRITS survey. We detect 8 Type Ia and …

We present infrared (IR) photometry and spectroscopy of the Type II-P SN 2017eaw and its
progenitor in the nearby galaxy NGC 6946. Progenitor observations in the Ks band in four …

Massive stars can shed material via steady, line-driven winds, eruptive outflows, or mass
transfer onto a binary companion. In the case of single stars, the mass is deposited by the …

Young core-collapse supernovae with dense-wind progenitors may be able to accelerate
cosmic-ray hadrons beyond the knee of the cosmic-ray spectrum, and this may result in …

We present the Supernova X-ray Database (SNaX), a compilation of the X-ray data from
young supernovae (SNe). The database includes the X-ray fluxes and luminosities of young …

We present a detailed compilation and analysis of the X-ray phase space of low-to
intermediate-redshift (0≤ z≤ 1) transients that consolidates observed light curves (and …