Showing 1–20 of 27 results
/ Date/ Name
Jun 9, 2023The Optical Corrector for the Dark Energy Spectroscopic InstrumentOct 27, 2025AT2025ulz and S250818k: Leveraging DESI spectroscopy in the hunt for a kilonova associated with a sub-solar mass gravitational wave candidateJan 18, 2026The DESI Transients Survey: Legacy Classifications and MethodologyJan 21, 2026Signatures of a Tidally Induced Spiral Arm at the Anticenter of the Milky Way and a Kinematically Extended Anticenter Stream Using DESI DR2Aug 12, 2025Measurement of Parity-Violating Modes of the Dark Energy Spectroscopic Instrument (DESI) Year 1 Luminous Red Galaxies' 4-Point Correlation FunctionNov 21, 2025Effect of local environment on Ly$α$ line profile in DESI/ODIN LAEsSep 24, 2025Dwarf galaxy halo masses from spectroscopic and photometric lensing in DESI and DESDec 1, 2025The Milky Way stellar halo is twisted and doubly broken: insights from DESI DR2 Milky Way Survey observationDec 17, 2025Cosmological Constraints from Full-Scale Clustering and Galaxy-Galaxy Lensing with DESI DR1Nov 28, 2025Baryon fraction from the BAO amplitude: a consistent approach to parameterizing perturbation growthNov 14, 2025ODIN: Characterizing the Three-dimensional Structure of Two Protocluster Complexes at $z = 3.1$Apr 2, 2026The velocity field of our Milky Way outer stellar halo based on DESI DR2Nov 3, 2025Quasars acting as Strong Lenses Found in DESI DR1Dec 17, 2025The Power of DESI for Photometric Redshift Calibration: A Case Study with KiDS-1000Jul 3, 2025The dark matter content of Milky Way dwarf spheroidal galaxies: Draco, Sextans and Ursa MinorDec 4, 2025The Binary Fraction of Stars in the Dwarf Galaxy Ursa Minor via Dark Energy Spectroscopic InstrumentMar 6, 2026Extremely Metal-Poor Galaxies in DESI DR1: Connections to Galaxies in the Early UniverseMar 26, 2026Nonlinear Information from DESI Luminous Red Galaxies: An Emulator-Based Analysis of Pre- and Post-Reconstruction Power SpectraApr 2, 2009BigBOSS: The Ground-Based Stage IV Dark Energy ExperimentOct 9, 2025Enhancing Multiplet Alignment Measurements with Imaging