학술논문
Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+Planck CMB weak lensing
Document Type
article
Author
Omori, Y; Baxter, EJ; Chang, C; Kirk, D; Alarcon, A; Bernstein, GM; Bleem, LE; Cawthon, R; Choi, A; Chown, R; Crawford, TM; Davis, C; De Vicente, J; DeRose, J; Dodelson, S; Eifler, TF; Fosalba, P; Friedrich, O; Gatti, M; Gaztanaga, E; Giannantonio, T; Gruen, D; Hartley, WG; Holder, GP; Hoyle, B; Huterer, D; Jain, B; Jarvis, M; Krause, E; MacCrann, N; Miquel, R; Prat, J; Rau, MM; Reichardt, CL; Rozo, E; Samuroff, S; Sánchez, C; Secco, LF; Sheldon, E; Simard, G; Troxel, MA; Vielzeuf, P; Wechsler, RH; Zuntz, J; Abbott, TMC; Abdalla, FB; Allam, S; Annis, J; Avila, S; Aylor, K; Benson, BA; Bertin, E; Bridle, SL; Brooks, D; Burke, DL; Carlstrom, JE; Rosell, A Carnero; Kind, M Carrasco; Carretero, J; Castander, FJ; Chang, CL; Cho, H-M; Crites, AT; Crocce, M; Cunha, CE; da Costa, LN; de Haan, T; Desai, S; Diehl, HT; Dietrich, JP; Dobbs, MA; Everett, WB; Fernandez, E; Flaugher, B; Frieman, J; García-Bellido, J; George, EM; Gruendl, RA; Gutierrez, G; Halverson, NW; Harrington, NL; Hollowood, DL; Honscheid, K; Holzapfel, WL; Hou, Z; Hrubes, JD; James, DJ; Jeltema, T; Kuehn, K; Kuropatkin, N; Lima, M; Lin, H; Lee, AT; Leitch, EM; Luong-Van, D; Maia, MAG; Manzotti, A; Marrone, DP; Marshall, JL; Martini, P
Source
Physical Review D. 100(4)
Subject
Language
Abstract
We cross-correlate galaxy weak lensing measurements from the Dark Energy Survey (DES) year-one data with a cosmic microwave background (CMB) weak lensing map derived from South Pole Telescope (SPT) and Planck data, with an effective overlapping area of 1289 deg2. With the combined measurements from four source galaxy redshift bins, we obtain a detection significance of 5.8σ. We fit the amplitude of the correlation functions while fixing the cosmological parameters to a fiducial ΛCDM model, finding A=0.99±0.17. We additionally use the correlation function measurements to constrain shear calibration bias, obtaining constraints that are consistent with previous DES analyses. Finally, when performing a cosmological analysis under the ΛCDM model, we obtain the marginalized constraints of ωm=0.261-0.051+0.070 and S8σ8ωm/0.3=0.660-0.100+0.085. These measurements are used in a companion work that presents cosmological constraints from the joint analysis of two-point functions among galaxies, galaxy shears, and CMB lensing using DES, SPT, and Planck data.