The mexico uk sub-mm camera for astronomy (muscat) on-sky commissioning: performance of the cryogenic systems

T. L.R. Brien, S. Doyle, D. H. Hughes, P. A.R. Ade, P. S. Barry, E. Castillo-Dominguez, C. Dodd, C. Dunscombe, S. Eales, D. Ferrusca, V. Gomez-Rivera, P. Hargrave, J. L. Hernandez-Rebollar, A. Hornsby, J. House, J. M. Jauregui-Garcia, P. D. Mauskopf, D. Murias, A. Papageorgiou, E. PascaleN. Peretto, A. Perez-Fajardo, S. Rowe, D. Sanchez-Arguelles, M. W.L. Smith, K. Souccar, R. Sudiwala, M. Tapia, A. T. Campos, C. Tucker, Rosa Becerra M. De La Velazquez, S. Ventura-Gonzalez, I. Walker

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

MUSCAT is a new 1.1 mm band receiver which was installed on the 50 m Large Millimeter Telescope atop Volcan Sierra Negra in Puebla, Mexico during the final quarter of 2021 and commissioned on sky throughout 2022. MUSCAT uses a novel cooling chain consisting of a commercial pulse tube cooler, two thermal stages of passively-switched continuous sorption coolers, and a final miniature dilution refrigerator. Through this system MUSCAT achieves a continuous temperature of 120 mK at the focal plane and has shown continuous operation at this temperature for greater than 100 days during readiness testing. Through minimising the amount of helium-3 required, the design on MUSCAT's cryogenic systems produced a reliable, cost-effective cooling platform. Here we present the cryogenic design and performance of MUSCAT on-sky and compare this to that achieved during deployment-readiness testing at Cardiff (UK). We consider both cooldown time and achieved base temperature. We look at the impact on operation of relocating a pulse-tube cooled instrument from a development lab running on a 50 Hz mains electricity supply to a site running at 60 Hz. Finally, we describe the process of preparing the MUSCAT instrument for shipping and assess the success of this process in terms of remedial work required upon arrival.

Original languageEnglish (US)
Title of host publicationMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI
EditorsJonas Zmuidzinas, Jian-Rong Gao
PublisherSPIE
ISBN (Electronic)9781510653610
DOIs
StatePublished - 2022
EventMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022 - Montreal, Canada
Duration: Jul 17 2022Jul 22 2022

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume12190
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022
Country/TerritoryCanada
CityMontreal
Period7/17/227/22/22

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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