Site Quality Analysis for an Indian Submillimeter Telescope: A Reanalysis-Based Approach
Tanmay Singh, Mayuri Sathyanarayana Rao, and Ritoban Basu Thakur

TL;DR
This study reanalyzes atmospheric data to identify promising sites in Ladakh, India, for a potential submillimeter telescope, highlighting two locations with favorable water vapor conditions compared to existing sites.
Contribution
It introduces a reanalysis-based approach using ECMWF ERA5 data to evaluate site suitability for submillimeter astronomy in Ladakh, India.
Findings
Two promising sites in Ladakh reach PWV ≤ 1 mm for 19-23% of the time.
Ladakh sites outperform Hanle and Merak in terms of PWV conditions.
The study provides transmittance and noise estimates over 10-1000 GHz.
Abstract
The Himalayan plateau region of Ladakh, India, is a potential host for a science-class submillimeter observatory, building on existing astronomical infrastructure near Hanle and Merak. Using the fifth-generation European Centre for Medium-Range Weather Forecasts (ECMWF) Reanalysis (ERA5) data, we analyze precipitable water vapor (PWV) at monthly resolution over 184 months from January 2010 to April 2025, map PWV statistics across Ladakh, and identify candidate regions that reach PWV mm. For promising locations, we compute atmospheric transmittance and the corresponding atmospheric photon noise using the am (Atmospheric Model) radiative transfer code; we present transmittance and brightness temperature estimates over 10--1000 GHz and compare the inferred performance to sites hosting current or planned submillimeter facilities worldwide. We find Ladakh to be favorable for…
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