activity
20222026
most citedLow luminosity Type II supernovae -- IV. SN 2020cxd and SN 2021aai, at the edges of the sub-luminous supernovae class

32 citations · 200 across the 33 of their papers we have counts for

collaborators
Showing 2023Show all

5 papers · 1 filter

astro-ph.SR2023★ 16 cited

A seven-Earth-radius helium-burning star inside a 20.5-min detached binary

Jie Lin, Chengyuan Wu, Heran Xiong +28

Binary evolution theory predicts that the second common envelope (CE) ejection can produce low-mass (0.32-0.36 Msun) subdwarf B (sdB) stars inside ultrashort-orbital-period binary…

astro-ph.HE2023

Detailed spectrophotometric analysis of the superluminous and fast evolving SN 2019neq

Achille Fiore, Stefano Benetti, Leonardo Tartaglia +24

SN 2019neq was a very fast evolving superluminous supernova. At a redshift z=0.1059, its peak absolute magnitude was -21.5+/-0.2 mag in g band. In this work, we present data and an…

astro-ph.HE2023

Strong Carbon Features and a Red Early Color in the Underluminous Type Ia SN 2022xkq

Jeniveve Pearson, David J. Sand, Peter Lundqvist +85

We present optical, infrared, ultraviolet, and radio observations of SN 2022xkq, an underluminous fast-declining type Ia supernova (SN Ia) in NGC 1784 ( Mpc),…

astro-ph.SR2023★ 29 cited

The broad-lined Type-Ic supernova SN 2022xxf with extraordinary two-humped light curves

H. Kuncarayakti, J. Sollerman, L. Izzo +60

We report on our study of supernova (SN) 2022xxf based on observations obtained during the first four months of its evolution. The light curves (LCs) display two humps of similar m…

astro-ph.HE2023★ 6 cited

Hidden shock powering the peak of SN 2020faa

I. Salmaso, E. Cappellaro, L. Tartaglia +9

The link between the fate of the most massive stars and the resulting supernova (SN) explosion is still a matter of debate, in major part because of the ambiguity among light-curve…