Showing 1–20 of 22 results
/ Date/ Name
Feb 6, 2025AT 2018dyk: tidal disruption event or active galactic nucleus? Follow-up observations of an extreme coronal line emitter with the Dark Energy Spectroscopic InstrumentNov 4, 2024The first identification of Lyman $α$ Changing-look Quasars at high-redshift in DESIMay 26, 2024ELG Spectroscopic Systematics Analysis of the DESI Data Release 1Apr 4, 2024High redshift LBGs from deep broadband imaging for future spectroscopic surveysApr 4, 2024Constraints on the spacetime variation of the fine-structure constant using DESI emission-line galaxiesNov 9, 2023A Spectroscopic Search for Optical Emission Lines from Dark Matter DecaySep 15, 2023The DESI One-Percent Survey: Evidence for Assembly Bias from Low-Redshift Counts-in-Cylinders MeasurementsJun 9, 2023Validation of semi-analytical, semi-empirical covariance matrices for two-point correlation function for Early DESI dataJun 9, 2023The DESI One-Percent Survey: Exploring A Generalized SHAM for Multiple Tracers with the UNIT SimulationMay 31, 2023Detecting and Characterizing Mg II absorption in DESI Survey Validation Quasar SpectraAug 17, 2022The Target-selection Pipeline for the Dark Energy Spectroscopic InstrumentJan 27, 2021Performance of the Dark Energy Spectroscopic Instrument(DESI) Fiber SystemAug 26, 2020Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clockJul 29, 2020Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the UniverseJul 5, 2020Dust Reverberation Mapping in Distant Quasars from Optical and Mid-Infrared Imaging SurveysMar 23, 2020Dark Energy Survey Identification of A Low-Mass Active Galactic Nucleus at Redshift 0.823 from Optical VariabilityFeb 25, 2020Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak LensingApr 24, 2019Spectral Variability of a Sample of Extreme Variability Quasars and Implications for the MgII Broad-line RegionJan 8, 2019The Buzzard Flock: Dark Energy Survey Synthetic Sky CatalogsSep 19, 2018Correcting for Fibre Assignment Incompleteness in the DESI Bright Galaxy Survey