activity
20052026
most citedAnalytical Light Curve Models of Super-Luminous Supernovae: chi^2-Minimizations of Parameter Fits

263 citations · 862 across the 22 of their papers we have counts for

collaborators

21 papers

astro-ph.SR2026

SN 2026dix: a nearby, transitional Type IIb/Ib supernova consistent with a warm supergiant progenitor

Tamás Szalai, Schuyler D. Van Dyk, Dominik Bánhidi +20

Understanding the final evolution stages of (very) massive stars and their explosive outcomes, stripped-envelope supernovae (SESNe), represent a long-term challenge for astrophysic…

astro-ph.HE2025

SN 2023ixf in M101: physical parameters from bolometric light curve modeling

J. Vinko, Zs. R. Bodola, A. Godeny +25

We present new photometric observations of the core-collapse supernova SN 2023ixf occurred in M101, taken with the RC80 and BRC80 robotic telescopes in Hungary. The initial nickel…

astro-ph.SR2023★ 7 cited

Three is the magic number -- distance measurement of NGC 3147 using SN 2021hpr and its siblings

Barnabas Barna, Andrea P. Nagy, Zsofia Bora +15

The nearby spiral galaxy NGC 3147 hosted three Type Ia supernovae (SNe Ia) in the past decades, which have been subjects of intense follow-up observations. Simultaneous analysis of…

astro-ph.HE2022

How to solve the mass-discrepancy problem of SESNe -- I. Testing model approximations

Andrea P. Nagy

Here, we present a systematic study of 59 stripped-envelope supernovae (SESNe) (including Type IIb, Ib, Ic, and transitional events) to map a possible reason for the so-called mass…

astro-ph.HE2022

SN 2019va: A Type IIP Supernova with Large Influence of Nickel-56 Decay on the Plateau-phase Light Curve

Xinghan Zhang, Xiaofeng Wang, Hanna Sai +12

We present multi-band photometric and spectroscopic observations of the type II supernova, (SN) 2019va, which shows an unusually flat plateau-phase evolution in its V-band light cu…

astro-ph.HE2021★ 9 cited

Rescued from oblivion: detailed analysis of archival {\it Spitzer} data of SN~1993J

Sz. Zsíros, A. P. Nagy, T. Szalai

We present an extensive analysis of the late-time mid-infrared (mid-IR) evolution of Type IIb SN 1993J from 10 up to 26 years post-explosion based on archival mostly previously…