Cosmological Constraints from Galaxy Clustering and Weak Lensing

By D. C. T. Abbott, Filipe B. Abdalla, A. Alarcon, J. Aleksi'c, Sahar Allam, S. Allen, Adam Amara, James Annis, J. Asorey, S. Ávila and 189 more. 2018

865 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/27a8dd1d488dc89527987c9b9917e7a6c63db084

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Citations in the corpus

• Constraining early dark energy with large-scale structure (2020, methodology): “Similarly, the combination of Dark Energy Survey (DES) [19] data and BOSS BAO data gives H0 = 67.”
• CMB-S4 Science Case, Reference Design, and Project Plan (2019, methodology): “, RSDs from the Baryon Oscillation Spectroscopic Survey (BOSS), Mν < 230 meV [227], and < 260 meV from DES lensing and galaxy clustering [228].”
• KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear (2019, methodology): “We note that the spectroscopically calibrated source redshift distributions will have a comparable impact on the S 8 constraint from the DES-Y1 combined analysis of cosmic shear, galaxy-galaxy lensing, and galaxy clustering (Abbott et al. 2018a).”
• Interacting dark energy in the early 2020s: A promising solution to the H0 and cosmic shear tensions (2019, methodology): “lensing likelihoods from the Dark Energy Survey (DES ) [5, 117, 118], the Planck collabo-”
• hmcode-2020: improved modelling of non-linear cosmological power spectra with baryonic feedback (2020, background): “…is constrainable by current weak-lensing surveys such as KiDS (e.g., Hildebrandt et al. 2020; Asgari et al. 2020; Heymans et al. 2020), DES (e.g., Abbott et al. 2018), or HSC (e.g., 2 Taken from the node cosmologies of Heitmann et al. (2014) and Lawrence et al. (2017) MNRAS 000, 1–17…”
• The cosmological analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure (2019, methodology): “18hMpc−1 respectively (left), and with the inclusion of the sound horizon prior (right), together with the same quantities from Planck2018 [83] and DES1Yr [87].”
• First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters (2018, background): “Ten 2.7 deg2 fields were observed approximately once per week in the griz filter bands (Abbott et al. 2018).”
• Measurements of the E -mode polarization and temperature- E -mode correlation of the CMB from SPT-3G 2018 data (2021, background): “5σ lower than the Dark Energy Survey (DES) Year 1 results [71] and 0.”
• Cosmology Intertwined II: The Hubble Constant Tension (2020, unknown): “[10] DES Collaboration, T.”