A comparative analysis of GNSS-inferred precipitable water vapour at the potential sites for the Africa Millimetre Telescope
Lott Frans, Michael Backes, Heino Falcke, and Tiziana Venturi

TL;DR
This study compares atmospheric water vapor at potential sites for the Africa Millimetre Telescope using GNSS data, finding Gamsberg Mountain has lower PWV and better conditions for millimetre observations than the H.E.S.S. site.
Contribution
It provides a comparative analysis of PWV conditions at two potential sites for the Africa Millimetre Telescope using GNSS data, identifying the more suitable location.
Findings
Gamsberg Mountain has lower median PWV than H.E.S.S.
Both sites are suitable for 86 and 230 GHz observations.
Gamsberg Mountain is the most suitable site due to lower PWV.
Abstract
The Event Horizon Telescope (EHT) is a network of antennas across the globe currently used to image super-massive black holes (SMBHs) at a frequency of 230 GHz. Since the release of the image of M87 in 2019 and, subsequently, that of Sgr A in 2022 by the EHT collaboration, the focus has shifted to dynamically imaging SMBHs. This has led to a search for potential sites to extend and fill in the gaps within the EHT network. The Gamsberg Mountain and the H.E.S.S. site are both located within the Khomas highlands and have been identified as potential sites for the Africa Millimetre Telescope (AMT). Precipitable water vapour (PWV) in the atmosphere is the main source of opacity and noise from atmospheric emissions when observing at millimetre to sub-millimetre wavelengths. This study aims to establish the PWV content and the atmospheric transmission at 86, 230, and 345 GHz at…
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