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arXiv · 2608.20235

The SPT-3G+ receiver design

H. Athreya·Z. Ahmed·J. E. Austermann·K. Bae·A. Bapat·D. R. Barron·P. S. Barry·A. N. Bender·B. A. Benson·L. E. Bleem·J. E. Carlstrom·T. W. Cecil·C. L. Chang·S. Cisneros·A. Coerver·J. Cornelison·R. Datta·K. R. Dibert·W. Dominguez·S. M. Duff·K. Fichman·J. P. Filippini·L. Gades·P. A. Gallardo·S. Galli·N. W. Halverson·Q. Hao·S. Henderson·R. Herbst·W. L. Holzapfel·A. Hryciuk·J. Hubmayr·D. Jones·V. Kabra·K. S. Karkare·C. King·M. A. Koc·A. M. Kofman·R. A. Lew·M. J. Link·T. J. Lucas·A. Mangu·E. S. Martsen·J. J. McMahon·J. Montgomery·J. M. Nagy·T. Natoli·H. Nguyen·V. Novosad·S. Padin·T. Pinsonneault-Marotte·S. Raghunathan·A. S. Rahlin·C. L. Reichardt·L. Ruckman·J. E. Ruhl·M. S. Sarwar·S. Simon·R. Singh·J. A. Sobrin·A. A. Stark·Q. Taylor·C. Tucker·J. Ullom·J. Van Lanen·J. D. Vieira·A. G. Vieregg·M. R. Vissers·G. Wang·W. L. K. Wu·V. Yefremenko·E. Yilmaz·C. Yu·J. Zivick
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Abstract

We present the thermo-mechanical design of the cryostat and camera optics for SPT-3G+, a new receiver being developed for the South Pole Telescope (SPT). The receiver consists of 14 detector arrays of 90/150 GHz dichroic polarization-sensitive pixels, totaling 24,080 transition-edge sensor detectors. Each detector array lies at the end of an optics tube, each approximately 240 mm in diameter and 772 mm in length, which are arranged in a hexagonal close-packed configuration to achieve a 4 degree diameter field of view. Each optics tube contains four anti-reflection coated lenses fabricated from different materials (alumina, silicon, and nylon) that are designed to also provide infrared filtering that reduces the radiative loading on the cryogenic stages. The optics and detectors are cooled by a combination of a pulse tube cooler for the 40 K and 4 K stages, and a dilution refrigerator for the 1 K and 100 mK stages. Thermal modeling predicts the heat load to be less than 26 W and 1 W for the 40 K and 4 K stages, respectively. The 1,550 kg cryostat has a 1.1 meter diameter at the vacuum window, which is located near the telescope Gregorian focus, and 1.75 meters in height and length. Fabrication of the cryostat will begin in 2026, with installation on the SPT scheduled for the 2028-29 austral summer, ahead of the 2029 winter observing season.

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H. Athreya, Z. Ahmed, J. E. Austermann, K. Bae, A. Bapat, D. R. Barron, P. S. Barry, A. N. Bender, B. A. Benson, L. E. Bleem, J. E. Carlstrom, T. W. Cecil, C. L. Chang, S. Cisneros, A. Coerver, J. Cornelison, R. Datta, K. R. Dibert, W. Dominguez, S. M. Duff, K. Fichman, J. P. Filippini, L. Gades, P. A. Gallardo, S. Galli, N. W. Halverson, Q. Hao, S. Henderson, R. Herbst, W. L. Holzapfel, A. Hryciuk, J. Hubmayr, D. Jones, V. Kabra, K. S. Karkare, C. King, M. A. Koc, A. M. Kofman, R. A. Lew, M. J. Link, T. J. Lucas, A. Mangu, E. S. Martsen, J. J. McMahon, J. Montgomery, J. M. Nagy, T. Natoli, H. Nguyen, V. Novosad, S. Padin, T. Pinsonneault-Marotte, S. Raghunathan, A. S. Rahlin, C. L. Reichardt, L. Ruckman, J. E. Ruhl, M. S. Sarwar, S. Simon, R. Singh, J. A. Sobrin, A. A. Stark, Q. Taylor, C. Tucker, J. Ullom, J. Van Lanen, J. D. Vieira, A. G. Vieregg, M. R. Vissers, G. Wang, W. L. K. Wu, V. Yefremenko, E. Yilmaz, C. Yu, J. Zivick. 2026-08-20. The SPT-3G+ receiver design. https://arxiv.org/abs/2608.20235

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