TY  - JOUR
AU  - Antoranz Canales, Pedro
AU  - Barrio Uña, Juan Abel
AU  - Contreras González, José Luis
AU  - Fonseca González, María Victoria
AU  - López Moya, Marcos
AU  - Miranda Pantoja, José Miguel
AU  - Satalecka, Konstanzja
AU  - Scapin, Valeria
PY  - 2014
DO  - 10.1051/0004-6361/201424261
SN  - 0004-6361
UR  - https://hdl.handle.net/20.500.14352/33900
T2  - Astronomy & Astrophysics
AB  - Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E >100 GeV) γ-ray source candidates. It is energized by one of the highest spin-down power pulsars known (5% of Crab pulsar) and it has been compared with the...
LA  - eng
PB  - EDP Sciencies
KW  - Supernova Remnant 3C-58
KW  - Large-area telescope
KW  - Spectral evolution
KW  - Constraints
KW  - Expansion
KW  - Distance
KW  - Catalog
KW  - Model.
TI  - Discovery of TeV gamma-ray emission from the pulsar wind nebula 3C 58 by MAGIC
TY  - journal article
VL  - 567
ER  -