Global Site Selection for Astronomy
N. Aksaker, S.K. Yerli, M.A. Erdo\u{g}an, Z. Kurt, K. Kaba, M., Bayazit, C. Yesilyaprak

TL;DR
This study developed a global suitability index for astronomical site selection using satellite data and multi-criteria analysis, identifying optimal regions and providing a web-based database for future observatory planning.
Contribution
Introduced the SIAS index for evaluating astronomical site suitability, integrating multiple satellite datasets and providing a practical tool for site selection.
Findings
Less than 3% of Earth's surface is ideal for observatories.
Only about 10% of existing observatories are in optimal locations.
Identified mid-western Andes and Tibetan Plateau as top sites.
Abstract
A global site selection for astronomy was performed with 1 km spatial resolution ( 1 Giga pixel in size) using long term and up-to-date datasets to classify the entire terrestrial surface on the Earth. Satellite instruments are used to get the following datasets of Geographical Information System (GIS) layers: Cloud Coverage, Digital Elevation Model, Artificial Light, Precipitable Water Vapor, Aerosol Optical Depth, Wind Speed and Land Use -- Land Cover. A Multi Criteria Decision Analysis (MCDA) technique is applied to these datasets creating four different series where each layer will have a specific weight. We introduce for the first time a ``Suitability Index for Astronomical Sites'' namely, SIAS. This index can be used to find suitable locations and to compare different sites or observatories. Mid-western Andes in South America and Tibetan Plateau in west China were found to…
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