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The dark energy survey supernova pro- gram: Light curves and 5-year data release

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it

fields

astro-ph.CO 4

years

2026 1 2025 3

representative citing papers

Probing Dark Energy Microphysics with kSZ Tomography

astro-ph.CO · 2025-11-07 · conditional · novelty 5.0

Fisher-matrix forecasts for LSST- and CMB-S4-like surveys show kSZ tomography tightens constraints on dark energy parameters w0 and wa by 15% and 32% while assessing detectability of perturbations for different sound speeds.

New Insights into Dark Energy from DESI DR2 with CMB and SNIa

astro-ph.CO · 2025-07-14 · unverdicted · novelty 4.0

Systematic dataset swaps show DESY5 low-redshift SNIa, Planck CMB plus lensing, and DESI-DR2 BAO as the dominant sources of w0waCDM tension with ΛCDM, while other combinations remain consistent.

Cosmic Strings as Dynamical Dark Energy: Novel Constraints

astro-ph.CO · 2025-05-28 · conditional · novelty 4.0

Cosmic string networks are constrained to less than ~1% of the energy density using CMB+BAO+SN data, with some models preferring mildly negative densities but no Bayesian evidence favoring them over LambdaCDM.

citing papers explorer

Showing 4 of 4 citing papers.

  • Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey astro-ph.CO · 2026-05-26 · unverdicted · none · ref 57

    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%.

  • Probing Dark Energy Microphysics with kSZ Tomography astro-ph.CO · 2025-11-07 · conditional · none · ref 67

    Fisher-matrix forecasts for LSST- and CMB-S4-like surveys show kSZ tomography tightens constraints on dark energy parameters w0 and wa by 15% and 32% while assessing detectability of perturbations for different sound speeds.

  • New Insights into Dark Energy from DESI DR2 with CMB and SNIa astro-ph.CO · 2025-07-14 · unverdicted · none · ref 8

    Systematic dataset swaps show DESY5 low-redshift SNIa, Planck CMB plus lensing, and DESI-DR2 BAO as the dominant sources of w0waCDM tension with ΛCDM, while other combinations remain consistent.

  • Cosmic Strings as Dynamical Dark Energy: Novel Constraints astro-ph.CO · 2025-05-28 · conditional · none · ref 80

    Cosmic string networks are constrained to less than ~1% of the energy density using CMB+BAO+SN data, with some models preferring mildly negative densities but no Bayesian evidence favoring them over LambdaCDM.