Dark Energy Survey Year 6 results: Redshift calibration of the MagLim++ lens sample
G. Giannini, A. Alarcon, W. d’Assignies, G. M. Bernstein et autres
es, us, de, mx, fr, it, br, ch, gb, au, tw, in, ca, ru, dk, se (code pays fourni par la source)
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G. Giannini, A. Alarcon, W. d’Assignies, G. M. Bernstein et autres
es, us, de, mx, fr, it, br, ch, gb, au, tw, in, ca, ru, dk, se (code pays fourni par la source)
G. Giannini, A. Alarcon, W d'Assignies, G. M. Bernstein et autres
In this work, we derive and calibrate the redshift distribution of the MagLim++ lens galaxy sample used in the Dark Energy Survey Year 6 (DES Y6) 3x2pt cosmology analysis. The 3x2pt analysis combines galaxy clustering from the lens galaxy sample and weak …
fr (code pays fourni par la source)
A. Porredon, M. Crocce, J. Elvin-Poole, R. Cawthon et autres
The cosmological information extracted from photometric surveys is most robust when multiple probes of the large scale structure of the Universe are used. Two of the most sensitive probes are the clustering of galaxies and the tangential shear of background galaxy shapes …
es, us, br, no, ch, gb, jp, cl, fr, it, au, in, de (code pays fourni par la source)
H. Camacho, F. Andrade-Oliveira, A. Troja, R. Rosenfeld et autres
ABSTRACT We perform a cosmic shear analysis in harmonic space using the first year of data collected by the Dark Energy Survey (DES-Y1). We measure the cosmic weak lensing shear power spectra using the metacalibration catalogue and perform a likelihood analysis within …
br, us, gb, ch, es, de, cl, fr, it, in, no, au (code pays fourni par la source)
Joseph DeRose, Risa H. Wechsler, M. R. Becker, E. S. Rykoff et autres
We present a validation of the Dark Energy Survey Year 3 (DES Y3) $3\ifmmode\times\else\texttimes\fi{}2$-point analysis choices by testing them on Buzzard2.0, a new suite of cosmological simulations that is tailored for the testing and validation of combined galaxy clustering and weak-lensing analyses. …
us, gb, ch, es, br, it, in, de, no, au (code pays fourni par la source)
C. Sánchez, J. Prat, Georgios Zacharegkas, Shivam Pandey et autres
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale galaxy-galaxy lensing measurements around the same lens sample to constrain source redshift uncertainties, intrinsic alignments and other systematics or nuisance parameters of our model. …
us, ch, gb, jp, br, es, de, cl, fr, it, in, no (code pays fourni par la source)
J. Prat, J. Blazek, C. Sánchez, I. Tutusaus et autres
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of data from the Dark Energy Survey (DES Y3) covering $4132\text{ }\text{ }{\mathrm{deg}}^{2}$. These galaxy-galaxy measurements are used in the DES Y3 $3\ifmmode\times\else\texttimes\fi{}2\text{ }\text{ }\mathrm{pt}$ cosmological analysis, which …
us, ch, es, gb, jp, de, br, pt, ca, cl, it, in (code pays fourni par la source)
Jesse B. Golden-Marx, C. J. Miller, Y. Zhang, R. L. C. Ogando et autres
Abstract We quantify evolution in the cluster-scale stellar mass–halo mass (SMHM) relation’s parameters using 2323 clusters and brightest central galaxies (BCGs) over the redshift range 0.03 ≤ z ≤ 0.60. The precision on the inferred SMHM parameters is improved by including the …
cn, us, br, cl, gb, fr, es, it, in, no, ch, au, de (code pays fourni par la source)
T. M. C. Abbott, M. Aguena, A. Alarcon, S. Allam et autres
We present the first cosmology results from large-scale structure using the full 5000 deg 2 of imaging data from the Dark Energy Survey (DES) Data Release 1.We perform an analysis of large-scale structure combining three two-point correlation functions (3 × 2pt): (i) …
cl, br, us, es, gb, ch, it, au, in, de, fr, ru, no, pt, ca (code pays fourni par la source)
L. F. Secco, S. Samuroff, E. Krause, Bhuvnesh Jain et autres
This work and its companion paper, Amon et al. [Phys. Rev. D 105, 023514 (2022)], present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the Dark Energy Survey (DES) Year 3 data. We constrain the lensing amplitude …
us, ch, gb, pt, ca, br, es, de, ru, fr, jp, cl (code pays fourni par la source)
A. Amon, D. Gruen, M. A. Troxel, N. MacCrann et autres
This work, together with its companion paper, Secco, Samuroff et al. [Phys. Rev. D 105, 023515 (2022)], present the Dark Energy Survey Year 3 cosmic-shear measurements and cosmological constraints based on an analysis of over 100 million source galaxies. With the data …
us, gb, br, ch, es, pt, ca, jp, de, fr, it (code pays fourni par la source)
E. Krause, Joseph DeRose, N. MacCrann, Bhuvnesh Jain et autres
We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clustering and galaxy-galaxy lensing measurements from the Dark Energy Survey (DES) year-3 data. We describe our modeling framework and choice of scales analyzed, validating their robustness to theoretical uncertainties in …
us, gb, es, ch, jp, br, de, cl, fr, it (code pays fourni par la source)
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