23 July 2014 SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope
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We describe the design of a new polarization sensitive receiver, spt-3g, for the 10-meter South Pole Telescope (spt). The spt-3g receiver will deliver a factor of ~20 improvement in mapping speed over the current receiver, spt-pol. The sensitivity of the spt-3g receiver will enable the advance from statistical detection of B-mode polarization anisotropy power to high signal-to-noise measurements of the individual modes, i.e., maps. This will lead to precise (~0.06 eV) constraints on the sum of neutrino masses with the potential to directly address the neutrino mass hierarchy. It will allow a separation of the lensing and inflationary B-mode power spectra, improving constraints on the amplitude and shape of the primordial signal, either through spt-3g data alone or in combination with bicep2/keck, which is observing the same area of sky. The measurement of small-scale temperature anisotropy will provide new constraints on the epoch of reionization. Additional science from the spt-3g survey will be significantly enhanced by the synergy with the ongoing optical Dark Energy Survey (des), including: a 1% constraint on the bias of optical tracers of large-scale structure, a measurement of the differential Doppler signal from pairs of galaxy clusters that will test General Relativity on ~200Mpc scales, and improved cosmological constraints from the abundance of clusters of galaxies
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B. A. Benson, B. A. Benson, P. A. R. Ade, P. A. R. Ade, Z. Ahmed, Z. Ahmed, S. W. Allen, S. W. Allen, K. Arnold, K. Arnold, J. E. Austermann, J. E. Austermann, A. N. Bender, A. N. Bender, L. E. Bleem, L. E. Bleem, J. E. Carlstrom, J. E. Carlstrom, C. L. Chang, C. L. Chang, H. M. Cho, H. M. Cho, J. F. Cliche, J. F. Cliche, T. M. Crawford, T. M. Crawford, A. Cukierman, A. Cukierman, T. de Haan, T. de Haan, M. A. Dobbs, M. A. Dobbs, D. Dutcher, D. Dutcher, W. Everett, W. Everett, A. Gilbert, A. Gilbert, N. W. Halverson, N. W. Halverson, D. Hanson, D. Hanson, N. L. Harrington, N. L. Harrington, K. Hattori, K. Hattori, J. W. Henning, J. W. Henning, G. C. Hilton, G. C. Hilton, G. P. Holder, G. P. Holder, W. L. Holzapfel, W. L. Holzapfel, K. D. Irwin, K. D. Irwin, R. Keisler, R. Keisler, L. Knox, L. Knox, D. Kubik, D. Kubik, C. L. Kuo, C. L. Kuo, A. T. Lee, A. T. Lee, E. M. Leitch, E. M. Leitch, D. Li, D. Li, M. McDonald, M. McDonald, S. S. Meyer, S. S. Meyer, J. Montgomery, J. Montgomery, M. Myers, M. Myers, T. Natoli, T. Natoli, H. Nguyen, H. Nguyen, V. Novosad, V. Novosad, S. Padin, S. Padin, Z. Pan, Z. Pan, J. Pearson, J. Pearson, C. Reichardt, C. Reichardt, J. E. Ruhl, J. E. Ruhl, B. R. Saliwanchik, B. R. Saliwanchik, G. Simard, G. Simard, G. Smecher, G. Smecher, J. T. Sayre, J. T. Sayre, E. Shirokoff, E. Shirokoff, A. A. Stark, A. A. Stark, K. Story, K. Story, A. Suzuki, A. Suzuki, K. L. Thompson, K. L. Thompson, C. Tucker, C. Tucker, K. Vanderlinde, K. Vanderlinde, J. D. Vieira, J. D. Vieira, A. Vikhlinin, A. Vikhlinin, G. Wang, G. Wang, V. Yefremenko, V. Yefremenko, K. W. Yoon, K. W. Yoon, } "SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope", Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 91531P (23 July 2014); doi: 10.1117/12.2057305; https://doi.org/10.1117/12.2057305

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