Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing
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...
Published in: | Physical Review D |
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Online Access: | http://www.osti.gov/servlets/purl/1574366 https://www.osti.gov/biblio/1574366 https://doi.org/10.1103/PhysRevD.100.043517 |
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ftosti:oai:osti.gov:1574366 2023-07-30T04:06:52+02:00 Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing Omori, Y. Baxter, E. J. Chang, C. Kirk, D. Alarcon, A. Bernstein, G. M. Bleem, L. E. Cawthon, R. Choi, A Chown, R. Chang, C. L. Carlstrom, J. E. Vikram, V. 2022-05-27 application/pdf http://www.osti.gov/servlets/purl/1574366 https://www.osti.gov/biblio/1574366 https://doi.org/10.1103/PhysRevD.100.043517 unknown http://www.osti.gov/servlets/purl/1574366 https://www.osti.gov/biblio/1574366 https://doi.org/10.1103/PhysRevD.100.043517 doi:10.1103/PhysRevD.100.043517 2022 ftosti https://doi.org/10.1103/PhysRevD.100.043517 2023-07-11T09:38:02Z 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 5.8 σ . We fit the amplitude of the correlation functions while fixing the cosmological parameters to a fiducial Λ CDM 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 Λ CDM model, we obtain the marginalized constraints of Ωm=0.26 1-0.051+0.070 and S8≡σ8√{Ωm/0.3 }=0.66 0-0.100+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. Other/Unknown Material South pole SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) South Pole Physical Review D 100 4 |
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SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) |
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description |
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 5.8 σ . We fit the amplitude of the correlation functions while fixing the cosmological parameters to a fiducial Λ CDM 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 Λ CDM model, we obtain the marginalized constraints of Ωm=0.26 1-0.051+0.070 and S8≡σ8√{Ωm/0.3 }=0.66 0-0.100+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. |
author |
Omori, Y. Baxter, E. J. Chang, C. Kirk, D. Alarcon, A. Bernstein, G. M. Bleem, L. E. Cawthon, R. Choi, A Chown, R. Chang, C. L. Carlstrom, J. E. Vikram, V. |
spellingShingle |
Omori, Y. Baxter, E. J. Chang, C. Kirk, D. Alarcon, A. Bernstein, G. M. Bleem, L. E. Cawthon, R. Choi, A Chown, R. Chang, C. L. Carlstrom, J. E. Vikram, V. Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing |
author_facet |
Omori, Y. Baxter, E. J. Chang, C. Kirk, D. Alarcon, A. Bernstein, G. M. Bleem, L. E. Cawthon, R. Choi, A Chown, R. Chang, C. L. Carlstrom, J. E. Vikram, V. |
author_sort |
Omori, Y. |
title |
Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing |
title_short |
Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing |
title_full |
Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing |
title_fullStr |
Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing |
title_full_unstemmed |
Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope+ Planck CMB weak lensing |
title_sort |
dark energy survey year 1 results: cross-correlation between dark energy survey y1 galaxy weak lensing and south pole telescope+ planck cmb weak lensing |
publishDate |
2022 |
url |
http://www.osti.gov/servlets/purl/1574366 https://www.osti.gov/biblio/1574366 https://doi.org/10.1103/PhysRevD.100.043517 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
http://www.osti.gov/servlets/purl/1574366 https://www.osti.gov/biblio/1574366 https://doi.org/10.1103/PhysRevD.100.043517 doi:10.1103/PhysRevD.100.043517 |
op_doi |
https://doi.org/10.1103/PhysRevD.100.043517 |
container_title |
Physical Review D |
container_volume |
100 |
container_issue |
4 |
_version_ |
1772819808178405376 |