69 citations · 236 across the 10 of their papers we have counts for
10 papers
Multiband Photometry Evolution in the First Weeks of SN 2023ixf, a possible II-L Subtype Supernova
Bianciardi G., Ciccarelli A. M., Conzo G. +8
Multiband photometric observations and their evaluation to instrumental magnitudes were performed using standard Johnson-Cousins filters (B, V, Rc) as well r and g Sloan filters, a…
Kepler Object of Interest Network III. Kepler-82f: A new non-transiting $21 M_\bigoplus$ planet from photodynamical modelling
J. Freudenthal, C. von Essen, A. Ofir +13
Context. The Kepler Object of Interest Network (KOINet) is a multi-site network of telescopes around the globe organised for follow-up observations of transiting planet candidate K…
Kepler Object of Interest Network II. Photodynamical modelling of Kepler-9 over 8 years of transit observations
J. Freudenthal, C. von Essen, S. Dreizler +14
The Kepler Object of Interest Network (KOINet) is a multi-site network of telescopes around the globe organised to follow up transiting planet candidate KOIs with large transit tim…
Diffuse γ-ray emission from self-confined cosmic rays around Galactic sources
M. D'Angelo, G. Morlino, E. Amato +1
The propagation of particles accelerated at supernova remnant shocks and escaping the parent remnants is likely to proceed in a strongly non-linear regime, due to the efficient sel…
Contribution to diffuse gamma-ray emission coming from self-confined CRs around their Galactic sources
G. Morlino, M. D'Angelo, P. Blasi +1
Recent observations of the diffuse Galactic gamma-ray emission by the Fermi-LAT satellite have shown significant deviations from models which assume the same diffusion properties f…
Do Cosmic Rays Heat the Early Intergalactic Medium?
Natacha Leite, Carmelo Evoli, Marta D'Angelo +3
Cosmic rays (CRs) govern the energetics of present-day galaxies and might have also played a pivotal role during the Epoch of Reionization. In particular, energy deposition by low-…
Grammage of cosmic rays around Galactic supernova remnants
Marta D'Angelo, Pasquale Blasi, Elena Amato
The residence time of cosmic rays (CRs) in the Galaxy is usually inferred from the measurement of the ratio of secondary-to-primary nuclei, such as the boron (B)/carbon (C) ratio,…
Extragalactic cosmic ray self-confinement around sources
P. Blasi, E. Amato, M. D'Angelo
Most models of the origin of ultra high energy cosmic rays rely on the existence of luminous extragalactic sources. Cosmic rays escaping the galaxy where the source is located prod…
High energy cosmic ray self-confinement close to extragalactic sources
P. Blasi, E. Amato, M. D'Angelo
The ultra-high energy cosmic rays observed at the Earth are most likely accelerated in extra-galactic sources. For the typical luminosities invoked for such sources, the electric c…
Particle acceleration and radiation friction effects in the filamentation instability of pair plasmas
M. D'Angelo, L. Fedeli, A. Sgattoni +2
The evolution of the filamentation instability produced by two counter-streaming pair plasmas is studied with particle-in-cell (PIC) simulations in both one (1D) and two (2D) spati…