Showing 1–20 of 33 results
/ Date/ Name
Jun 4, 2025A Correlation Between FRB Dispersion Measure and Foreground Large-Scale StructureMay 9, 2023Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case StudiesApr 26, 2023A ring-like accretion structure in M87 connecting its black hole and jetDec 8, 2022System Design for an Integrated Lifelong Reinforcement Learning Agent for Real-Time Strategy GamesMar 17, 2022The Dwarf Galaxy Population at $z\sim 0.7$: A Catalog of Emission Lines and Redshifts from Deep Keck ObservationsJan 18, 2022WATCH: Wasserstein Change Point Detection for High-Dimensional Time Series DataSep 24, 2021The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3Sep 2, 2020CANDELS Meets GSWLC: Evolution of the Relationship Between Morphology and Star Formation Since z = 2Jun 25, 2020Stellar Masses of Giant Clumps in CANDELS and Simulated Galaxies Using Machine LearningAug 21, 2019Structural and Stellar Population Properties vs. Bulge Types in Sloan Digital Sky Survey Central GalaxiesNov 8, 2018Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshiftsMay 2, 2018On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELSDec 4, 2017Spatially resolved kinematics in the central 1 kpc of a compact star-forming galaxy at z=2.3 from ALMA CO observationsOct 16, 2017Demographics of Star-forming Galaxies since $z\sim2.5$. I. The $UVJ$ Diagram in CANDELSMay 15, 2017UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profilesMar 1, 2017The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBCOct 10, 2016Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELSSep 3, 2014Galaxy Zoo: CANDELS Barred Disks and Bar FractionsJul 28, 2014No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HSTJun 20, 2013CANDELS: The correlation between galaxy morphology and star formation activity at z~2