Showing 1–20 of 139 results
/ Date/ Name
May 20, 2009Coexistence of Weak Ferromagnetism and Ferroelectricity in the High Pressure LiNbO3-type Phase of FeTiO3Oct 25, 2009Continuous metal-insulator transition of the antiferromagnetic perovskite NaOsO3Jul 12, 2022A galaxy-driven model of type Ia supernova luminosity variationsFeb 16, 2022Robust sampling for weak lensing and clustering analyses with the Dark Energy SurveyOct 25, 2018Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol DataJan 29, 2020Increasing the census of L and T dwarfs in wide binary and multiple systems using Dark Energy Survey DR1 and Gaia DR2 dataJul 18, 2018Modeling projection effects in optically-selected cluster cataloguesDec 10, 2020A machine learning approach to galaxy properties: joint redshift-stellar mass probability distributions with Random ForestOct 12, 2018Balancing polyhedraMar 21, 2019Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clustersMay 25, 2020Is diffuse intracluster light a good tracer of the galaxy cluster matter distribution?Mar 23, 2020The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveysSep 8, 2021A search of the full six years of the Dark Energy Survey for outer Solar System objectsFeb 20, 2021Synthetic Galaxy Clusters and Observations Based on Dark Energy Survey Year 3 DataOct 22, 2018Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSSAug 4, 2017Dark Energy Survey Year 1 Results: Weak Lensing Shape CataloguesMar 4, 2024Dark Energy Survey Year 3 results: likelihood-free, simulation-based $w$CDM inference with neural compression of weak-lensing map statisticsFeb 13, 2024The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy ClustersOct 19, 2021Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass mapsOct 5, 2021The DES Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5,000 Sq. Deg. Footprint