Abstract Type Ia supernovae (SNe Ia) play a key role in the fields of astrophysics and
cosmology. It is widely accepted that SNe Ia arise from thermonuclear explosions of white …

We present a JWST/MIRI low-resolution mid-infrared (MIR) spectroscopic observation of the
normal Type Ia supernova (SN Ia) SN 2021aefx at+ 323 days past rest-frame B-band …

We present JWST near-infrared (NIR) and mid-infrared (MIR) spectroscopic observations of
the nearby normal Type Ia supernova (SN) SN 2021aefx in the nebular phase at+ 255 days …

We present 307 type Ia supernova (SN) light curves from the first 4 yr of the Transiting
Exoplanet Survey Satellite mission. We use this sample to characterize the shapes of the …

We present a photometric and spectroscopic analysis of the ultraluminous and slowly
evolving 03fg-like Type Ia SN 2021zny. Our observational campaign starts from∼ 5.3 h after …

ABSTRACT Type Ia supernovae (SNe Ia) arise from the thermonuclear explosion in binary
systems involving carbon–oxygen white dwarfs (WDs). The pathway of WDs acquiring mass …

Context. Recent JWST observations of the Type Ia supernova (SN Ia) 2021aefx in the
nebular phase have paved the way for late-time studies covering the full optical to mid …

We present ultraviolet (UV) to near-infrared (NIR) observations and analysis of the nearby
Type Ia supernova SN 2021fxy. Our observations include UV photometry from Swift/UVOT …

SN 2018aoz is a Type Ia SN with a B-band plateau and excess emission in infant-phase
light curves≲ 1 day after the first light, evidencing an over-density of surface iron-peak …

SN 2021aefx is a normal Type Ia supernova (SN) showing excess emission and redward
color evolution over the first∼ 2 days. We present analyses of this SN using our high …