We use the light-curve and spectral synthesis code JEKYLL to calculate a set of
macroscopically mixed type IIb supernova (SN) models, which are compared to both …

We present optical, near-infrared, and radio observations of supernova (SN) SN IIb 2022crv.
We show that it retained a very thin H envelope and transitioned from an SN IIb to an SN Ib; …

Nitrogen is produced by CNO-cycling in massive stars, and can be ejected in significant
amounts in supernova explosions. While in H-rich SNe, its [N ii] 6548, 6583 emission …

ABSTRACT The Near Infrared (NIR) spectra of the Type IIb supernova (SN IIb) SN 2020acat,
obtained at various times throughout the optical follow-up campaign, are presented here …

We present photometric and spectroscopic observations and analysis of the Type IIb
supernova (SN) SN 2019tua, which exhibits multiple bumps in its declining light curves …

We present the discovery and analysis of SN 2022oqm, a Type Ic supernova (SN) detected<
1 day after the explosion. The SN rises to a blue and short-lived (2 days) initial peak. Early …

We present the discovery and analysis of SN\, 2022oqm, a Type Ic supernova (SN) detected
$< 1$\, day after explosion. The SN rises to a blue and short-lived (2\, days) initial peak …

Aims. Stripped envelope (SE) supernovae are explosions of stars that have somehow lost
most of their outer envelopes. We present the discovery and analyse the observations of the …

We use the light-curve and spectral synthesis code JEKYLL to calculate a set of
macroscopically mixed type IIb supernova (SN) models, which are compared to both …

Massive stars, with 𝑀ZAMS> 8 M⊙, end their lives as explosive events known as
corecollapse supernovae (CC-SNe). A sub-class of these CC-SNe have had some or part of …