activity
20032024
most citedModeling of proton-induced radioactivation background in hard X-ray telescopes: Geant4-based simulation and its demonstration by Hitomi's measurement in a low Earth orbit

18 citations · 50 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2024

A new air shower array in the Southern Hemisphere looking for the origins of Cosmic rays: the ALPACA experiment

M. Anzorena, E. de la Fuente, K. Fujita +53

The Tibet AS experiment successfully detected sub-PeV -rays from the Crab nebula using a Surface Array and underground muon detector. Considering this, we are building in Bol…

astro-ph.HE2023★ 1 cited

Small-scale cosmic ray anisotropy observed by the GRAPES-3 experiment at TeV energies

M. Chakraborty, S. Ahmad, A. Chandra +35

GRAPES-3 is a mid-altitude (2200 m) and near equatorial ( North) air shower array, overlapping in its field of view for cosmic ray observations with experiments that…

astro-ph.SR2022

Proton Penetration Efficiency over a High Altitude Observatory in Mexico

S. Miyake, T. Koi, Y. Muraki +12

In association with a large solar flare on November 7, 2004, the solar neutron detectors located at Mt. Chacaltaya (5,250m) in Bolivia and Mt. Sierra Negra (4,600m) in Mexico recor…

astro-ph.HE2021★ 18 cited

Detectability of southern gamma-ray sources beyond 100 TeV with ALPAQUITA, the prototype experiment of ALPACA

S. Kato, C. A. H. Condori, E. dela Fuente +47

Andes Large-area PArticle detector for Cosmic-ray physics and Astronomy (ALPACA) is an international experiment that applies southern very-high-energy (VHE) gamma-ray astronomy to…

astro-ph.SR2020★ 3 cited

Solar Neutron Decay Protons observed in November 7, 2004

Yasushi Muraki, Jose F. Valde-Galicia, Ernesto Ortiz +10

We have found an interesting event registered by the solar neutron telescopes installed at high mountains in Bolivia (5250 m a.s.l.) and Mexico (4600 m a.s.l.). The event was obser…

astro-ph.IM2020★ 3 cited

Origin of the in-orbit instrumental background of the Hard X-ray Imager onboard Hitomi

Kouichi Hagino, Hirokazu Odaka, Goro Sato +43

Understanding and reducing the in-orbit instrumental backgrounds are essential to achieving high sensitivity in hard X-ray astronomical observations. The observational data of the…