The Thirty Meter Telescope (TMT) must remove waste heat generated by electronics on the telescope to prevent overheating and reduce their impact on dome seeing. Traditionally, chilled water-glycol cooling loops have been used for this purpose. However, the potential (and realization on existing telescopes) for damage and disruption due to glycol leaks at the telescope top end has prompted a shift to a refrigerant system, where any leaking refrigerant vaporizes immediately. Additionally, a refrigerant system is needed to cool adaptive optics enclosures to -30°C and cool the telescope hydrostatic bearing oil to -21°C, below the operating range of a chilled water system. This paper discusses the refrigerant services infrastructure in development for the observatory, including the cooling requirements, the trade study that led to the choice of carbon dioxide as the refrigerant, the conceptual design, and the concept of operations.
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