Showing 1–20 of 21 results
/ Date/ Name
Feb 20, 2026dfcosmic: A Python package for cosmic ray removalJul 25, 2025JWST+ALMA reveal the build up of stellar mass in the cores of dusty star-forming galaxies at Cosmic NoonMay 6, 2025dfreproject: A Python package for astronomical reprojectionApr 4, 2025Investigating the Ultra-diffuse Galaxy NGC5846_UDG1 through the Kinematics of its Rich Globular Cluster SystemDec 1, 2024Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-Field ImagesJun 25, 2024Realizing the potential of the Dragonfly Spectral Line Mapper: Calibration methods and on-sky performanceFeb 8, 2024UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at $z_{spec}=3.97$Nov 27, 2023The Heavy Metal Survey: Star Formation Constraints and Dynamical Masses of 21 Massive Quiescent Galaxies at $z=1.3-2.3$Sep 5, 2023Accelerated Formation of Ultra-Massive Galaxies in the First Billion YearsJul 5, 2023Dust attenuation, dust content and geometry of star-forming galaxiesJun 13, 2023A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical ImagesAug 4, 2022Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?Aug 2, 2022JWST reveals a population of ultra-red, flattened disk galaxies at 2<z<6 previously missed by HSTApr 12, 2022Light from the Darkness: Detecting Ultra-Diffuse Galaxies in the Perseus Cluster through Over-densities of Globular Clusters with a Log-Gaussian Cox ProcessMar 9, 2022A giant shell of ionized gas discovered near M82 with the Dragonfly Spectral Line Mapper pathfinderApr 15, 2020Measuring distances to low-luminosity galaxies using surface brightness fluctuationsOct 30, 2019The Dragonfly Wide Field Survey. I. Telescope, Survey Design and Data CharacterizationOct 11, 2019The Dragonfly Edge-on Galaxies Survey: Shaping the outer disc of NGC 4565 via accretionMar 22, 2017KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7Mar 3, 2016The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D