Year: 2026
Type: preprint
Abstract: This article aims to raise awareness within the ESO astronomical community of the scientific opportunities offered by the upcoming Cherenkov Telescope Array Observatory (CTAO), highlighting cases where combining the millimetre/submillimetre capabilities of the Atacama Large Millimeter/submillimeter Array (ALMA) with the CTAO’s very-high-energy (~TeV) observations enables new avenues for discovery. Many astrophysical sources and environments exhibit emission processes detectable in both regimes; however, the synergies extend beyond shared emission mechanisms and include broader physical processes and observational connections linking millimetre/submillimetre and TeV energies.
Source: arXiv (Cornell University)
Authors: Andreani, Paola, Díaz Trigo, María
Institutions: European Southern Observatory, European Southern Observatory
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W7165531510