Showing 1–17 of 17 results
/ Date/ Name
Mar 23, 2026Little Red and Blue Dots: simply stratified Broad Line RegionsJan 29, 2026The Little Blue and Red Dots Rosetta Stones: Non-Gaussian broad lines, hot dust, and X-ray weaknessJan 13, 2026RotCurves: A PYTHON package for efficient modelling and fitting of galactic rotation curves at high-zMay 9, 2025The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studiesMar 2, 2025A large-scale ring galaxy at z = 2.2 revealed by JWST/NIRCam: kinematic observations and analytical modellingDec 5, 2024The radio properties of the JWST-discovered AGNJul 12, 2024The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at z=5.66Apr 16, 2024New AGN diagnostic diagrams based on the [OIII]$λ4363$ auroral lineMay 4, 2023Evidence for Large-scale, Rapid Gas Inflows in z~2 Star-forming DisksNov 15, 2022A ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259Sep 25, 2022RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic ScalesJul 13, 2022Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic SystemsMar 1, 2022Kiloparsec view of a typical star-forming galaxy when the Universe was $\sim$1 Gyr old II. Regular rotating disk and evidence for baryon dominance on galactic scalesSep 6, 2021Rotation Curves in z~1-2 Star-Forming Disks: Comparison of Dark Matter Fractions and Disk Properties for Different Fitting MethodsDec 18, 2020The KMOS$^{\rm 3D}$ Survey: Investigating the Origin of the Elevated Electron Densities in Star-Forming Galaxies at $1\lesssim{z}\lesssim{3}$Jun 4, 2020Rotation Curves in z~1-2 Star-Forming Disks: Evidence for Cored Dark Matter DistributionsApr 6, 2020From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI