TY  - GEN 
AU  - Fiore, Achille
AU  - Benetti, Stefano
AU  - Tartaglia, Leonardo
AU  - Jerkstrand, Anders
AU  - Salmaso, Irene
AU  - Tomasella, Lina
AU  - Morales Garoffolo, Antonia Isabel
AU  - Geier, Stefan
AU  - Elias-Rosa, Nancy
AU  - Cappellaro, Enrico
AU  - Wang, Xiaofeng
AU  - Mo, Jun
AU  - Chen, Zhihao
AU  - Yan, Shengyu
AU  - Pastorello, Andrea
AU  - Mazzali, Paolo A.
AU  - Ciolfi, Riccardo
AU  - Cai, Yongzhi
AU  - Fraser, Morgan
AU  - Gutiérrez, Claudia P.
AU  - Karamehmetoglu, Emir
AU  - Kuncarayakti, Hanindyo
AU  - Moran, Shane
AU  - Ochner, Paolo
AU  - Reguitti, Andrea
AU  - Reynolds, T. M.
AU  - Valerin, Giorgio
A4  - Física Aplicada
PY  - 2024
SN  - 1365-2966
SN  - 0035-8711
UR  - http://hdl.handle.net/10498/31753
AB  - 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 analysis from an extensive spectrophotometric follow-up campaign using...
LA  - eng
PB  - Oxford University Press
KW  - supernovae
KW  - general –supernovae
KW  - individual
KW  - SN 2019neq
TI  - Detailed spectrophotometric analysis of the superluminous and fast evolving SN 2019neq
DO  - 10.1093/mnras/stad3655
ER  -