Design and Performance of the SPT-SLIM Receiver Cryostat

Fuente: arXiv
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Main Authors: Young, M. R., Adamic, M., Anderson, A. J., Barry, P. S., Benson, B. A., Benson, C. S., Brooks, E., Carlstrom, J. E., Cecil, T., Chang, C. L., Dibert, K. R., Dobbs, M., Fichman, K., Hollister, M., Karkare, K. S., Keating, G. K., Lapuente, A. M., Lisovenko, M., Marrone, D. P., Mitchell, D., Montgomery, J., Natoli, T., Pan, Z., Rahlin, A., Robson, G., Rouble, M., Smecher, G., Yefremenko, V., Yu, C., Zebrowski, J. A., Zhang, C.
Format: Preprint
Published: 2025
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author Young, M. R.
Adamic, M.
Anderson, A. J.
Barry, P. S.
Benson, B. A.
Benson, C. S.
Brooks, E.
Carlstrom, J. E.
Cecil, T.
Chang, C. L.
Dibert, K. R.
Dobbs, M.
Fichman, K.
Hollister, M.
Karkare, K. S.
Keating, G. K.
Lapuente, A. M.
Lisovenko, M.
Marrone, D. P.
Mitchell, D.
Montgomery, J.
Natoli, T.
Pan, Z.
Rahlin, A.
Robson, G.
Rouble, M.
Smecher, G.
Yefremenko, V.
Yu, C.
Zebrowski, J. A.
Zhang, C.
author_facet Young, M. R.
Adamic, M.
Anderson, A. J.
Barry, P. S.
Benson, B. A.
Benson, C. S.
Brooks, E.
Carlstrom, J. E.
Cecil, T.
Chang, C. L.
Dibert, K. R.
Dobbs, M.
Fichman, K.
Hollister, M.
Karkare, K. S.
Keating, G. K.
Lapuente, A. M.
Lisovenko, M.
Marrone, D. P.
Mitchell, D.
Montgomery, J.
Natoli, T.
Pan, Z.
Rahlin, A.
Robson, G.
Rouble, M.
Smecher, G.
Yefremenko, V.
Yu, C.
Zebrowski, J. A.
Zhang, C.
contents The South Pole Telescope Shirokoff Line Intensity Mapper (SPT-SLIM) is a millimeter-wavelength line-intensity mapping experiment, which was deployed on the South Pole Telescope (SPT) during the 2024-2025 Austral summer season. This pathfinder experiment serves to demonstrate the on-sky operation of multi-pixel on-chip spectrometer technology. We report on the cryogenic performance of the SPT-SLIM receiver for the first year of commissioning observations. The SPT-SLIM receiver utilizes an Adiabatic Demagnetization Refrigerator (ADR) for cooling the focal plane of superconducting filterbank spectrometers to a temperature of 150 mK. We demonstrate stable thermal performance of the focal plane module during observations consistent with thermal modeling, enabling a cryogenic operating efficiency above 80%. We also report on the receiver control system design utilizing the Observatory Control System (OCS) platform for automated cryogenic operation on the SPT.
format Preprint
id arxiv_https___arxiv_org_abs_2510_14219
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Design and Performance of the SPT-SLIM Receiver Cryostat
Young, M. R.
Adamic, M.
Anderson, A. J.
Barry, P. S.
Benson, B. A.
Benson, C. S.
Brooks, E.
Carlstrom, J. E.
Cecil, T.
Chang, C. L.
Dibert, K. R.
Dobbs, M.
Fichman, K.
Hollister, M.
Karkare, K. S.
Keating, G. K.
Lapuente, A. M.
Lisovenko, M.
Marrone, D. P.
Mitchell, D.
Montgomery, J.
Natoli, T.
Pan, Z.
Rahlin, A.
Robson, G.
Rouble, M.
Smecher, G.
Yefremenko, V.
Yu, C.
Zebrowski, J. A.
Zhang, C.
Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
The South Pole Telescope Shirokoff Line Intensity Mapper (SPT-SLIM) is a millimeter-wavelength line-intensity mapping experiment, which was deployed on the South Pole Telescope (SPT) during the 2024-2025 Austral summer season. This pathfinder experiment serves to demonstrate the on-sky operation of multi-pixel on-chip spectrometer technology. We report on the cryogenic performance of the SPT-SLIM receiver for the first year of commissioning observations. The SPT-SLIM receiver utilizes an Adiabatic Demagnetization Refrigerator (ADR) for cooling the focal plane of superconducting filterbank spectrometers to a temperature of 150 mK. We demonstrate stable thermal performance of the focal plane module during observations consistent with thermal modeling, enabling a cryogenic operating efficiency above 80%. We also report on the receiver control system design utilizing the Observatory Control System (OCS) platform for automated cryogenic operation on the SPT.
title Design and Performance of the SPT-SLIM Receiver Cryostat
topic Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2510.14219