Dr. Emma de Ona Wilhelmi

Profil

Derzeitige StellungProfessor W-1 und Äquivalente
FachgebietAstrophysik
KeywordsCherenkov Telescopes, Pulsars and pulsar winds, High-energy astrophysics, Gamma-ray astronomy

Aktuelle Kontaktadresse

LandSpanien
OrtBarcelona
Universität/InstitutionICREA & Institut de Ciencies de L'Espai (IEEC-CSIC)

Gastgeber*innen während der Förderung

Prof. Dr. Christian StegmannPhoto Injector Test Facility (PITZ), Deutsches Elektronen-Synchrotron (DESY) Hamburg, Zeuthen
Beginn der ersten Förderung01.07.2018

Programm(e)

2017Humboldt-Forschungsstipendien-Programm für erfahrene Forschende

Publikationen (Auswahl)

2020Li, Jian and ... de Ona Wilhelmi, Emma: Gamma-ray heartbeat powered by the microquasar SS 433. In: Nature Astronomy, 2020,
2020de Ona Wilhelmi, Emma et al.: SNR G39.2-0.3, an hadronic cosmic rays accelerator. In: Monthly Notices of the Royal Astronomical Society, 497, 2020, 3581-3590
2020Mestre, E. and de Ona Wilhelmi et al.: {Prospects for the characterization of the VHE emission from the Crab nebula and pulsar with the Cherenkov Telescope Array}. In: Monthly Notices of the Royal Astronomical Society, 492, 2020, 708-718
2019Felix Aharonian, Ruizhi Yang, Emma de Oña Wilhelmi: Massive Stars as Major Factories of Galactic Cosmic Rays. In: Nature Astronomy, 2019, 561-567
2019CTA Consortium (+Emma de Ona Wilhelmi): Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout. In: Astroparticle Physics, 2019,
2019L. Ambrogi, R. Zanin, S. Casanova, E. De Ona Wilhelmi, G. Peron, F. Aharonian: Spectral and morphological study of the gamma radiation of the middle-aged supernova remnant HB 21. In: Astronomy and Astrophysics, 2019, A86
2019H.E.S.S. Collaboration (+ Emma de Ona Wilhelmi): Upper Limits on Very-High-Energy Gamma-ray Emission from Core-Collapse Supernovae Observed with H.E.S.S. In: Astronomy & Astrophysics, 2019,
2018MAGIC Collaboration (+Emma de Ona Wilhelmi): Discovery of TeV ?-ray emission from the neighbourhood of the supernova remnant G24.7+0.6 by MAGIC. In: MNRAS, 2018, 4578-4585