Next generation of IACT arrays: scientific objectives versus energy domains

TL;DR

This paper discusses the scientific goals and technical considerations for the next generation of Imaging Atmospheric Cherenkov Telescope (IACT) arrays across four key gamma-ray energy domains, aiming to advance ground-based gamma-ray astronomy.

Contribution

It provides an analysis of the scientific objectives and detection techniques tailored to four major gamma-ray energy ranges for future IACT arrays.

Findings

Identifies key scientific motivations for each energy domain.

Highlights technical challenges and detection strategies.

Outlines the potential scientific impact of next-generation IACTs.

Abstract

Several key motivations and perspectives of ground based gamma-ray astronomy are discussed in the context of the specifics of detection techniques and scientific topics/objectives relevant to four major energy domains -- very-low or \textit{multi-GeV} ($E \leq$ 30 GeV), low or \textit{sub-TeV} (30 GeV - 300 GeV), high or \textit{TeV} (300 GeV - 30 TeV), and very-high or \textit{sub-PeV} ($E \geq$ 30 TeV) intervals -- to be covered by the next generation of IACT arrays.