activity
20042026
most citedThe Type IIb Supernova 2011dh from a Supergiant Progenitor

245 citations · 3.2k across the 64 of their papers we have counts for

collaborators

63 papers

astro-ph.SR2026

The nearby Type II supernova 2024ggi beyond 600 days: circumstellar interaction and dust formation

L. Ferrari, G. Folatelli, C. P. Gutiérrez +16

The Type II SN 2024ggi is one of the nearest core-collapse SNe to have exploded in recent decades. Its proximity has enabled extensive multiwavelength monitoring from early times t…

astro-ph.SR2025★ 5 cited

The nebular phase of SN 2024ggi: a low-mass progenitor with no signs of interaction

L. Ferrari, G. Folatelli, K. Ertini +14

Context: SN 2024ggi is a Type II supernova (SN) discovered in the nearby galaxy NGC 3621 (D Mpc) on 2024 April 03.21 UT. Its proximity enabled a detailed investi…

astro-ph.HE2025

SN2022jli modeled with a Ni double-layer and a magnetar

Mariana Orellana, Melina C. Bersten, Claudia P. Gutiérrez

We study the bolometric evolution of the exceptional Type Ic Supernova (SN) 2022jli, aiming to understand the underlying mechanisms responsible for its distinctive double-peaked li…

astro-ph.HE2025★ 1 cited

Hydrodynamical modeling of SN 2025kg associated with the Fast X-ray Transient EP250108a

L. M. Roman Aguilar, M. C. Bersten

Supernovae (SNe) associated with X-Ray Flashes (XRFs) are extremely rare. Therefore, the discovery of each new object in this class offers a unique opportunity to improve our under…

astro-ph.HE2025★ 6 cited

A magnetar powers the luminous supernova 2023pel, associated with a long gamma-ray burst

L. M. Roman Aguilar, M. M. Saez, K. Ertini +1

We explore SN 2023pel, the most recent event associated with gamma-ray bursts (GRBs), specifically GRB 230812B. SN 2023pel has a high luminosity and low expansion velocities compar…

astro-ph.SR2025★ 5 cited

Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling

Arkaprabha Sarangi, Szanna Zsiros, Tamas Szalai +20

The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations after a few years from explosion. Most theories…