학술논문

A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
Document Type
Working Paper
Author
Pan, Z.Bianchini, F.Wu, W. L. K.Ade, P. A. R.Ahmed, Z.Anderes, E.Anderson, A. J.Ansarinejad, B.Archipley, M.Aylor, K.Balkenhol, L.Barry, P. S.Thakur, R. BasuBenabed, K.Bender, A. N.Benson, B. A.Bleem, L. E.Bouchet, F. R.Bryant, L.Byrum, K.Camphuis, E.Carlstrom, J. E.Carter, F. W.Cecil, T. W.Chang, C. L.Chaubal, P.Chen, G.Chichura, P. M.Cho, H. -M.Chou, T. -L.Cliche, J. -F.Coerver, A.Crawford, T. M.Cukierman, A.Daley, C.de Haan, T.Denison, E. V.Dibert, K. R.Ding, J.Dobbs, M. A.Doussot, A.Dutcher, D.Everett, W.Feng, C.Ferguson, K. R.Fichman, K.Foster, A.Fu, J.Galli, S.Gambrel, A. E.Gardner, R. W.Ge, F.Goeckner-Wald, N.Gualtieri, R.Guidi, F.Guns, S.Gupta, N.Halverson, N. W.Harke-Hosemann, A. H.Harrington, N. L.Henning, J. W.Hilton, G. C.Hivon, E.Holder, G. P.Holzapfel, W. L.Hood, J. C.Howe, D.Huang, N.Irwin, K. D.Jeong, O.Jonas, M.Jones, A.Kéruzoré, F.Khaire, T. S.Knox, L.Kofman, A. M.Korman, M.Kubik, D. L.Kuhlmann, S.Kuo, C. -L.Lee, A. T.Leitch, E. M.Levy, K.Lowitz, A. E.Lu, C.Maniyar, A.Menanteau, F.Meyer, S. S.Michalik, D.Millea, M.Montgomery, J.Nadolski, A.Nakato, Y.Natoli, T.Nguyen, H.Noble, G. I.Novosad, V.Omori, Y.Padin, S.Paschos, P.Pearson, J.Posada, C. M.Prabhu, K.Quan, W.Raghunathan, S.Rahimi, M.Rahlin, A.Reichardt, C. L.Riebel, D.Riedel, B.Ruhl, J. E.Sayre, J. T.Schiappucci, E.Shirokoff, E.Smecher, G.Sobrin, J. A.Stark, A. A.Stephen, J.Story, K. T.Suzuki, A.Takakura, S.Tandoi, C.Thompson, K. L.Thorne, B.Trendafilova, C.Tucker, C.Umilta, C.Vale, L. R.Vanderlinde, K.Vieira, J. D.Wang, G.Whitehorn, N.Yefremenko, V.Yoon, K. W.Young, M. R.Zebrowski, J. A.
Source
Physical Review D 108.12 (2023): 122005
Subject
Astrophysics - Cosmology and Nongalactic Astrophysics
Language
Abstract
We present a measurement of gravitational lensing over 1500 deg$^2$ of the Southern sky using SPT-3G temperature data at 95 and 150 GHz taken in 2018. The lensing amplitude relative to a fiducial Planck 2018 $\Lambda$CDM cosmology is found to be $1.020\pm0.060$, excluding instrumental and astrophysical systematic uncertainties. We conduct extensive systematic and null tests to check the robustness of the lensing measurements, and report a minimum-variance combined lensing power spectrum over angular multipoles of $50Comment: Bandpower and likelihood data available at https://pole.uchicago.edu/public/data/spt3g_2018_lensing/