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Dark Energy Survey Year 6 Results: Photometric Data Set for Cosmology

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arxiv 2501.05739 v2 pith:Z22U2R4J submitted 2025-01-10 astro-ph.CO

Dark Energy Survey Year 6 Results: Photometric Data Set for Cosmology

classification astro-ph.CO
keywords dataphotometricgoldcosmologymillionsurveyanalysesclassification
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We describe the photometric data set assembled from the full six years of observations by the Dark Energy Survey (DES) in support of static-sky cosmology analyses. DES Y6 Gold is a curated data set derived from DES Data Release 2 (DR2) that incorporates improved measurement, photometric calibration, object classification and value added information. Y6 Gold comprises nearly $5000~{\rm deg}^2$ of $grizY$ imaging in the south Galactic cap and includes 669 million objects with a depth of $i_{AB} \sim 23.4$ mag at S/N $\sim 10$ for extended objects and a top-of-the-atmosphere photometric uniformity $< 2~{\rm mmag}$. Y6 Gold augments DES DR2 with simultaneous fits to multi-epoch photometry for more robust galaxy shapes, colors, and photometric redshift estimates. Y6 Gold features improved morphological star-galaxy classification with efficiency $98.6\%$ and contamination $0.8\%$ for galaxies with $17.5 < i_{AB} < 22.5$. Additionally, it includes per-object quality information, and accompanying maps of the footprint coverage, masked regions, imaging depth, survey conditions, and astrophysical foregrounds that are used for cosmology analyses. After quality selections, benchmark samples contain 448 million galaxies and 120 million stars. This paper will be complemented by online data access and documentation.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey

    astro-ph.CO 2026-05 unverdicted novelty 6.0

    Full DES data from SN+BAO+3x2pt yields w0=-0.84, wa=-0.44 with 2.2σ deviation from ΛCDM; adding DESI+CMB reaches 3.0σ while 3x2pt improves figure of merit by ~10%.

  2. UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space

    astro-ph.CO 2026-05 accept novelty 5.0

    UNIONS-3500 weak lensing data yields S_8 = 0.831^{+0.067}_{-0.078} in flat LCDM from 2D cosmic shear, consistent with Planck within 1 sigma.

  3. Infrared-enhanced Photometric Redshifts for the Dark Energy Survey Y6 Gold catalogue

    astro-ph.CO 2026-07 accept novelty 4.0

    DES+WISE W1/W2 photometry significantly reduces photo-z scatter, bias and outliers versus optical-only DES, while VHS adds only marginal gains at z<1.5.

  4. GWTC-5.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    Analysis of 236 GW events from GWTC-5.0 constrains H0 to 71.0 +9.0/-7.1 km/s/Mpc and finds no evidence for modified gravitational-wave propagation.