scholarly journals Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty

2022 ◽  
Vol 105 (2) ◽  
Author(s):  
L. F. Secco ◽  
S. Samuroff ◽  
E. Krause ◽  
B. Jain ◽  
J. Blazek ◽  
...  
Keyword(s):  
Dark Energy ◽  
Modeling Uncertainty ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey

scholarly journals x -cut Cosmic shear: Optimally removing sensitivity to baryonic and nonlinear physics with an application to the Dark Energy Survey year 1 shear data

2021 ◽  
Vol 103 (4) ◽  
Author(s):  
Peter L. Taylor ◽  
Francis Bernardeau ◽  
Eric Huff
Keyword(s):  
Dark Energy ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey

scholarly journals KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear

2020 ◽  
Vol 638 ◽  
pp. L1 ◽  
Author(s):  
S. Joudaki ◽  
H. Hildebrandt ◽  
D. Traykova ◽  
N. E. Chisari ◽  
C. Heymans ◽  
...  
Keyword(s):  
Dark Energy ◽  
Cosmic Microwave Background ◽  
Gravitational Lensing ◽  
Error Model ◽  
Calibration Error ◽  
Microwave Background ◽  
Weak Gravitational Lensing ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey

We present a combined tomographic weak gravitational lensing analysis of the Kilo Degree Survey (KV450) and the Dark Energy Survey (DES-Y1). We homogenize the analysis of these two public cosmic shear datasets by adopting consistent priors and modeling of nonlinear scales, and determine new redshift distributions for DES-Y1 based on deep public spectroscopic surveys. Adopting these revised redshifts results in a 0.8σ reduction in the DES-inferred value for S​8, which decreases to a 0.5σ reduction when including a systematic redshift calibration error model from mock DES data based on the MICE2 simulation. The combined KV450+DES-Y1 constraint on S8 = 0.762−0.024+0.025 is in tension with the Planck 2018 constraint from the cosmic microwave background at the level of 2.5σ. This result highlights the importance of developing methods to provide accurate redshift calibration for current and future weak-lensing surveys.

scholarly journals Inference from the small scales of cosmic shear with current and future Dark Energy Survey data

2016 ◽  
Vol 465 (3) ◽  
pp. 2567-2583 ◽  
Author(s):  
N. MacCrann ◽  
J. Aleksić ◽  
A. Amara ◽  
S. L. Bridle ◽  
C. Bruderer ◽  
...  
Keyword(s):  
Dark Energy ◽  
Survey Data ◽  
Dark Energy Survey ◽  
Small Scales ◽  
Cosmic Shear ◽  
Energy Survey

scholarly journals Cosmic shear measurements with Dark Energy Survey Science Verification data

2016 ◽  
Vol 94 (2) ◽  
Author(s):  
M. R. Becker ◽  
M. A. Troxel ◽  
N. MacCrann ◽  
E. Krause ◽  
T. F. Eifler ◽  
...  
Keyword(s):  
Dark Energy ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey

scholarly journals Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration

2022 ◽  
Vol 105 (2) ◽  
Author(s):  
A. Amon ◽  
D. Gruen ◽  
M. A. Troxel ◽  
N. MacCrann ◽  
S. Dodelson ◽  
...  
Keyword(s):  
Dark Energy ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey ◽  
Data Calibration

scholarly journals KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs

2020 ◽  
Vol 634 ◽  
pp. A127 ◽  
Author(s):  
Marika Asgari ◽  
Tilman Tröster ◽  
Catherine Heymans ◽  
Hendrik Hildebrandt ◽  
Jan Luca van den Busch ◽  
...  
Keyword(s):  
Dark Energy ◽  
Mode Analysis ◽  
Small Scale ◽  
Microwave Background ◽  
Cosmological Constraints ◽  
Dark Energy Survey ◽  
Matter Power Spectrum ◽  
Λcdm Model ◽  
Cosmic Shear ◽  
Energy Survey

We present cosmological constraints from a joint cosmic shear analysis of the Kilo-Degree Survey (KV450) and the Dark Energy Survey (DES-Y1), which were conducted using Complete Orthogonal Sets of E/B-Integrals (COSEBIs). With COSEBIs, we isolated any B-modes that have a non-cosmic shear origin and demonstrate the robustness of our cosmological E-mode analysis as no significant B-modes were detected. We highlight how COSEBIs are fairly insensitive to the amplitude of the non-linear matter power spectrum at high k-scales, mitigating the uncertain impact of baryon feedback in our analysis. COSEBIs, therefore, allowed us to utilise additional small-scale information, improving the DES-Y1 joint constraints on S8 = σ8(Ωm/0.3)0.5 and Ωm by 20%. By adopting a flat ΛCDM model we find S8 = 0.755−0.021+0.019, which is in 3.2σ tension with the Planck Legacy analysis of the cosmic microwave background.

scholarly journals Cosmology from cosmic shear with Dark Energy Survey Science Verification data

2016 ◽  
Vol 94 (2) ◽  
Author(s):  
T. Abbott ◽  
F. B. Abdalla ◽  
S. Allam ◽  
A. Amara ◽  
J. Annis ◽  
...  
Keyword(s):  
Dark Energy ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey

scholarly journals Dark Energy Survey Year 1: An independent E/B-mode cosmic shear analysis

2019 ◽  
Vol 484 (1) ◽  
pp. L59-L63 ◽  
Author(s):  
Marika Asgari ◽  
Catherine Heymans
Keyword(s):  
Dark Energy ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey

scholarly journals Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear

2018 ◽  
Vol 98 (4) ◽  
Author(s):  
M. A. Troxel ◽  
N. MacCrann ◽  
J. Zuntz ◽  
T. F. Eifler ◽  
E. Krause ◽  
...  
Keyword(s):  
Dark Energy ◽  
Cosmological Constraints ◽  
Dark Energy Survey ◽  
Cosmic Shear ◽  
Energy Survey

scholarly journals A machine learning approach to the detection of ghosting and scattered light artifacts in dark energy survey images

2021 ◽  
pp. 100474
Author(s):  
C. Chang ◽  
A. Drlica-Wagner ◽  
S.M. Kent ◽  
B. Nord ◽  
D.M. Wang ◽  
...  
Keyword(s):  
Machine Learning ◽  
Dark Energy ◽  
Scattered Light ◽  
Learning Approach ◽  
Dark Energy Survey ◽  
Machine Learning Approach ◽  
Energy Survey
Sign in / Sign up

Export Citation Format

Share Document