Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 2019
DOI: 10.22323/1.358.0412
|View full text |Cite
|
Sign up to set email alerts
|

Modeling the LAGO's detectors response to secondary particles at ground level from the Antarctic to Mexico

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
5
0

Year Published

2019
2019
2022
2022

Publication Types

Select...
4
3

Relationship

1
6

Authors

Journals

citations
Cited by 7 publications
(5 citation statements)
references
References 21 publications
0
5
0
Order By: Relevance
“…The LAGO-ARTI framework allows us to estimate the response of the WCD to the cosmic ray background radiation flux (Ξ) at any site [45]. This toolkit employs a Geant4 code to estimate the number of Cherenkov photons detected by the PMT with its quantum efficiency.…”
Section: Wcd Response To the Cosmic Ray Background Radiationmentioning
confidence: 99%
“…The LAGO-ARTI framework allows us to estimate the response of the WCD to the cosmic ray background radiation flux (Ξ) at any site [45]. This toolkit employs a Geant4 code to estimate the number of Cherenkov photons detected by the PMT with its quantum efficiency.…”
Section: Wcd Response To the Cosmic Ray Background Radiationmentioning
confidence: 99%
“…Moreover, recent studies on regions in the CCD with low collection efficiency [15] show how large-energy ionization events could produce low-energy signals in the detector. For this reasons, experiments running above ground are more challenging due to the larger rate of atmospheric high-energy particles [16,17]. Several new low-threshold technologies observe a rapidly increasing rate of background events towards low energies (below 1 keV).…”
Section: Thick Fully Depleted Ccds For Particle Detection Experimentsmentioning
confidence: 99%
“…We adopted the LAGO-ARTI framework [9] to simulate the interaction between an IED and a cosmic ray background radiation flux at ground level. This computation framework considers three important factors with different spatial and time scales: the geomagnetic effects, the development of the extensive air showers in the atmosphere, and the detector response at ground level.…”
Section: Simulation Of the Interaction Between An Ied And Cosmic Radiationmentioning
confidence: 99%