It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample,
Paul Shah et al.,
Mon.Not.Roy.Astron.Soc. 537 (2025) 3814-3825,arXiv:2501.19117.
[DES:2025omh]
Constraints on compact objects from the Dark Energy Survey 5-yr supernova sample,
P. Shah et al.(DES),
Mon. Not. Roy. Astron. Soc. 536 (2025) 946-961,arXiv:2410.07956.
[DES:2024ffp]
The Dark Energy Survey: Cosmology Results With $\sim 1500$ New High-redshift Type Ia Supernovae Using The Full 5-year Dataset,
T. M. C. Abbott et al.(DES),
Astrophys.J.Lett. 973 (2024) L14,arXiv:2401.02929.
[DES:2024jxu]
Dark Energy Survey Year 3 Results: Constraints on extensions to $\Lambda$CDM with weak lensing and galaxy clustering,
T. M. C. Abbott et al.(DES),
Phys.Rev.D 107 (2023) 083504,arXiv:2207.05766.
[DES:2022ccp]
Dark energy survey year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space,
C. Doux et al.(DES),
Mon. Not. Roy. Astron. Soc. 515 (2022) 1942-1972,arXiv:2203.07128.
[DES:2022qpf]
Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State,
D. O. Jones et al.,
Astrophys. J. 933 (2022) 172,arXiv:2201.07801.
[Jones:2022mvo]
Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps,
M. Gatti et al.(DES),
Phys.Rev.D 106 (2022) 083509,arXiv:2110.10141.
[DES:2021lsy]
Dark energy survey year 3 results: Cosmology with peaks using an emulator approach,
D. Zurcher et al.(DES),
Mon. Not. Roy. Astron. Soc. 511 (2022) 2075-2104,arXiv:2110.10135.
[DES:2021epj]
Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations,
Juan P. Cordero et al.(DES),
Mon.Not.Roy.Astron.Soc. 511 (2022) 2170-2185,arXiv:2109.09636.
[DES:2021vvo]
Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement,
A. Carnero Rosell et al.(DES),
Mon.Not.Roy.Astron.Soc. 509 (2021) 778-799,arXiv:2107.05477.
[DES:2021jns]
Dark Energy Survey Year 3 Results: A 2.7\% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835,
T. M. C. Abbott et al.(DES),
Phys.Rev.D 105 (2022) 043512,arXiv:2107.04646.
[DES:2021esc]
Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis,
I. Ferrero et al.(DES),
Astron.Astrophys. 656 (2021) A106,arXiv:2107.04602.
[DES:2021fie]
Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing,
G. Zacharegkas et al.(DES),
Mon.Not.Roy.Astron.Soc. 509 () 3119-3147,arXiv:2106.08438.
[DES:2021olg]
Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing,
T. M. C. Abbott et al.(DES),
Phys.Rev.D 105 (2022) 023520,arXiv:2105.13549.
[DES:2021wwk]
Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing - validation on cosmological simulations,
J. DeRose et al.(DES),
Phys.Rev.D 105 (2022) 123520,arXiv:2105.13547.
[DES:2021bwg]
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample,
A. Porredon et al.(DES),
Phys.Rev.D 106 (2022) 103530,arXiv:2105.13546.
[DES:2021bpo]
Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample,
S. Pandey et al.(DES),
Phys.Rev.D 106 (2022) 043520,arXiv:2105.13545.
[DES:2021zxv]
Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty,
L. F. Secco et al.(DES),
Phys.Rev.D 105 (2022) 023515,arXiv:2105.13544.
[DES:2021vln]
Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration,
A. Amon et al.(DES),
Phys.Rev.D 105 (2022) 023514,arXiv:2105.13543.
[DES:2021bvc]
Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios,
Carles Sanchez et al.(DES),
Phys.Rev.D 105 (2022) 083529,arXiv:2105.13542.
[DES:2021jzg]
Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing,
J. Prat et al.(DES),
Phys.Rev.D 105 (2022) 083528,arXiv:2105.13541.
[DES:2021qnp]
Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples,
M. Rodriguez-Monroy et al.(DES),
Mon.Not.Roy.Astron.Soc. 511 (2022) 2665,arXiv:2105.13540.
[DES:2021bat]
Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction,
N. Jeffrey et al.(DES),
Mon. Not. Roy. Astron. Soc. 505 (2021) 4626-4645,arXiv:2105.13539.
[DES:2021gua]
Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS,
R. Cawthon et al.(DES),
Mon.Not.Roy.Astron.Soc. 513 (2022) 5517,arXiv:2012.12826.
[DES:2020sjz]
Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog,
S. Everett et al.(DES),
Astrophys.J.Supp. 258 (2022) 15,arXiv:2012.12825.
[DES:2020jnm]
Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and Catalogue,
W. G. Hartley et al.(DES),
Mon.Not.Roy.Astron.Soc. 509 (2021) 3547-3579,arXiv:2012.12824.
[DES:2020drs]
Dark Energy Survey Year 3 Results: Clustering Redshifts - Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS,
M. Gatti et al.(DES),
Mon.Not.Roy.Astron.Soc. 510 (2022) 1223-1247,arXiv:2012.08569.
[DES:2020rlj]
Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit,
O. Friedrich et al.(DES),
Mon.Not.Roy.Astron.Soc. 508 (2021) 3125-3165,arXiv:2012.08568.
[DES:2020ypx]
Dark Energy Survey Year 3 results: redshift calibration of the weak lensing source galaxies,
J. Myles et al.(DES),
Mon. Not. Roy. Astron. Soc. 505 (2021) 4249-4277,arXiv:2012.08566.
[DES:2020ebm]
Dark Energy Survey Year 3 results: Optimizing the lens sample in a combined galaxy clustering and galaxy-galaxy lensing analysis,
A. Porredon et al.(DES),
Phys. Rev. D 103 (2021) 043503,arXiv:2011.03411.
[DES:2020ajx]
Dark Energy Survey year 3 results: point spread function modelling,
M. Jarvis et al.(DES),
Mon. Not. Roy. Astron. Soc. 501 (2021) 1282-1299,arXiv:2011.03409.
[DES:2020vau]
Dark energy survey year 3 results: weak lensing shape catalogue,
M. Gatti et al.(DES),
Mon. Not. Roy. Astron. Soc. 504 (2021) 4312-4336,arXiv:2011.03408.
[DES:2020ekd]
Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology,
I. Sevilla-Noarbe et al.(DES),
Astrophys. J. Suppl. 254 (2021) 24,arXiv:2011.03407.
[DES:2020aks]
Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps - validation on simulations,
M. Gatti et al.(DES),
Mon. Not. Roy. Astron. Soc. 498 (2020) 4060-4087,arXiv:1911.05568.
[DES:2019ujq]
Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions,
T. Giannantonio et al.(DES),
Phys.Rev. D99 (2019) 023508,arXiv:1802.05257.
[DES:2018zzu]
Dark Energy Survey Year 1 Results: Calibration of redMaGiC Redshift Distributions in DES and SDSS from Cross-Correlations,
R. Cawthon et al.,
Mon.Not.Roy.Astron.Soc. 481 (2018) 2427,arXiv:1712.07298.
[DES:2017mbc]
Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO,
S. Avila et al.,
Mon.Not.Roy.Astron.Soc. 479 (2018) 94-110,arXiv:1712.06232.
[DES:2017ngw]
Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement,
M. Crocce et al.,
Mon.Not.Roy.Astron.Soc. 482 (2019) 2807-2822,arXiv:1712.06211.
[DES:2017odw]
Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1,
T. M. C. Abbott et al.(DES),
Mon.Not.Roy.Astron.Soc. 483 (2019) 4866-4883,arXiv:1712.06209.
[DES:2017rfo]
Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data,
T. M. C. Abbott et al.(DES),
Mon.Not.Roy.Astron.Soc. 480 (2018) 3879,arXiv:1711.00403.
[DES:2017txv]
Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear,
M. A. Troxel et al.(DES),
Phys.Rev. D98 (2018) 043528,arXiv:1708.01538.
[DES:2017qwj]
Dark Energy Survey Year 1 Results: Galaxy clustering for combined probes,
J. Elvin-Poole et al.(DES),
Phys.Rev. D98 (2018) 042006,arXiv:1708.01536.
[DES:2017hdw]
Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map,
C. Chang et al.(DES),
Mon.Not.Roy.Astron.Soc. 475 (2018) 3165,arXiv:1708.01535.
[DES:2017stf]
Dark Energy Survey Year 1 Results: The Impact of Galaxy Neighbours on Weak Lensing Cosmology with im3shape,
S. Samuroff et al.(DES),
Mon.Not.Roy.Astron.Soc. 475 (2018) 4524,arXiv:1708.01534.
[DES:2017ewg]
Dark Energy Survey Year 1 Results: Weak Lensing Shape Catalogues,
J. Zuntz et al.,
Mon.Not.Roy.Astron.Soc. 481 (2018) 1149-1182,arXiv:1708.01533.
[DES:2017ibv]
Dark Energy Survey Year 1 Results: Redshift distributions of the weak lensing source galaxies,
B. Hoyle et al.(DES),
Mon.Not.Roy.Astron.Soc. 478 (2018) 592-610,arXiv:1708.01532.
[DES:2017ndt]
Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology,
A. Drlica-Wagner et al.(DES),
Astrophys.J.Suppl. 235 (2018) 33,arXiv:1708.01531.
[DES:2017myt]
Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing,
T. M. C. Abbott et al.(DES),
Phys.Rev. D98 (2018) 043526,arXiv:1708.01530.
[DES:2017myr]
Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses,
E. Krause et al.(DES),
arXiv:1706.09359, 2017. [DES:2017tss]
Dark Energy Survey Year 3 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Clustering,
T. M. C. Abbott et al.(DES),
Phys.Rev.D 112 (2025) 083535,arXiv:2503.13632.
[DESCollaboration:2025udj]
Dark Energy Survey: implications for cosmological expansion models from the final DES Baryon Acoustic Oscillation and Supernova data,
T. M. C. Abbott et al.(DES),
Phys.Rev.D 113 (2026) 063530,arXiv:2503.06712.
[DES:2025upx]
Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing,
S. Bocquet et al.(DES, SPT),
Phys.Rev.D 111 (2025) 063533,arXiv:2412.07765.
[DES:2024viv]
Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data,
Asmaa Mazoun, Sebastian Bocquet, Joseph J. Mohr, Mathias Garny, Henrique Rubira, Matthias Klein, Lindsey Bleem, Sebastian Grandis, Tim Schrabback(SPT, DES),
Phys.Rev.D 111 (2025) 083543,arXiv:2411.19911.
[SPT:2024roj]
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