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  • Performance of Al–Mn Transi...
    Anderson, A. J.; Ade, P. A. R.; Ahmed, Z.; Avva, J. S.; Barry, P. S.; Thakur, R. Basu; Bender, A. N.; Benson, B. A.; Bryant, L.; Byrum, K.; Carlstrom, J. E.; Carter, F. W.; Cecil, T. W.; Chang, C. L.; Cho, H.-M.; Cliche, J. F.; Cukierman, A.; de Haan, T.; Denison, E. V.; Ding, J.; Dobbs, M. A.; Dutcher, D.; Everett, W.; Ferguson, K. R.; Foster, A.; Fu, J.; Gallicchio, J.; Gambrel, A. E.; Gardner, R. W.; Gilbert, A.; Groh, J. C.; Guns, S. T.; Guyser, R.; Halverson, N. W.; Harke-Hosemann, A. H.; Harrington, N. L.; Henning, J. W.; Hilton, G. C.; Holzapfel, W. L.; Howe, D.; Huang, N.; Irwin, K. D.; Jeong, O. B.; Jonas, M.; Jones, A.; Khaire, T. S.; Kofman, A. M.; Korman, M.; Kubik, D. L.; Kuhlmann, S.; Kuo, C.-L.; Lee, A. T.; Leitch, E. M.; Lowitz, A. E.; Meyer, S. S.; Michalik, D.; Montgomery, J.; Nadolski, A.; Natoli, T.; Nguyen, H.; Noble, G. I.; Novosad, V.; Padin, S.; Pan, Z.; Paschos, P.; Pearson, J.; Posada, C. M.; Quan, W.; Rahlin, A.; Riebel, D.; Ruhl, J. E.; Sayre, J. T.; Shirokoff, E.; Smecher, G.; Sobrin, J. A.; Stark, A. A.; Stephen, J.; Story, K. T.; Suzuki, A.; Thompson, K. L.; Tucker, C.; Vale, L. R.; Vanderlinde, K.; Vieira, J. D.; Wang, G.; Whitehorn, N.; Yefremenko, V.; Yoon, K. W.; Young, M. R.

    Journal of low temperature physics, 04/2020, Letnik: 199, Številka: 1-2
    Journal Article

    SPT-3G is a polarization-sensitive receiver, installed on the South Pole Telescope, that measures the anisotropy of the cosmic microwave background (CMB) from degree to arcminute scales. The receiver consists of ten 150-mm-diameter detector wafers, containing a total of ∼ 16 , 000 transition-edge sensor (TES) bolometers observing at 95, 150, and 220 GHz. During the 2018–2019 austral summer, one of these detector wafers was replaced by a new wafer fabricated with Al–Mn TESs instead of the Ti/Au design originally deployed for SPT-3G. We present the results of in-laboratory characterization and on-sky performance of this Al–Mn wafer, including electrical and thermal properties, optical efficiency measurements, and noise-equivalent temperature. In addition, we discuss and account for several calibration-related systematic errors that affect measurements made using frequency-domain multiplexing readout electronics.