activity
20102019
most citedMonte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

72 citations · 101 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2023

Tomographic Imaging of the Sagittarius Spiral Arm's Magnetic Field Structure

Yasuo Doi, Kengo Nakamura, Koji S. Kawabata +16

The Galactic global magnetic field is thought to play a vital role in shaping Galactic structures such as spiral arms and giant molecular clouds. However, our knowledge of magnetic…

astro-ph.IM201972 cited

Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

A. Acharyya, I. Agudo, E. O. Angüner +467

The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current groun…

astro-ph.HE20169 cited

Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps II: the effects of instabilities feedback

R. Santos-Lima, E. M. de Gouveia Dal Pino, D. A. Falceta-Gonçalves +2

Statistical analysis of Faraday Rotation Measure (RM) maps of the intracluster medium (ICM) of galaxy clusters provides a unique tool to evaluate some spatial features of the magne…

astro-ph.HE20161 cited

Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

The CTA Consortium, :, A. Abchiche +1387

List of contributions from the Cherenkov Telescope Array (CTA) Consortium presented at the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016), July 11-15,…

astro-ph.HE201418 cited

Runaway stars as cosmic ray injectors inside molecular clouds

Maria Victoria del Valle, Gustavo E. Romero, Reinaldo Santos-Lima

Giant molecular clouds (GMCs) are a new population of gamma-ray sources, being the target of cosmic rays (CRs) -- locally accelerated or not --. These clouds host very young stella…

astro-ph.GA20101 cited

Reconnection Diffusion and Star Formation

A. Lazarian, R. Santos-Lima, E. Gouveia Dal Pino

The diffusion of astrophysical magnetic fields in conducting fluids in the presence of turbulence depends on whether magnetic fields can change their topology or reconnect in highl…