Showing 121–140 of 2,473 results
/ Date/ Name
Nov 21, 2025Comparing galaxy merger orbits in hydrodynamical simulation and in dark-matter-only simulationNov 20, 2025A search for cold molecular outflows in cosmic noon galaxiesNov 19, 2025Do z>6 quasars reside in protoclusters?Nov 18, 2025Dynamics in the Cores of Self-Interacting Dark Matter Halos: Reduced Stalling and Accelerated Core CollapseNov 18, 2025Localized Deviations from the CO-PAH Relation in PHANGS-JWST Galaxies: Faint PAH Emission or Elevated CO Emissivity?Nov 18, 2025VENUS: A Strongly Lensed Clumpy Galaxy at $z\sim11-12$ behind the Galaxy Cluster MACS J0257.1-2325Nov 17, 2025JWST observes the assembly of a massive galaxy at z~4Nov 17, 2025Sense and Sensitivity - I. Uncertainty analysis of the gas-phase chemistry in AGB outflowsNov 17, 2025SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar materialNov 14, 2025Not all cores are equal: Phase-space origins of dynamical friction, stalling and buoyancyNov 13, 2025Large-Scale Structure in COSMOS-Web: Tracing Galaxy Evolution in the Cosmic Web up to $z \sim 7$ with the Largest JWST SurveyNov 11, 2025Where Giants Dwell: Probing the Environments of Early Massive Quiescent GalaxiesNov 5, 2025Peculiar galaxies I: A Catalog of Polar-Ring Galaxies from the TNG50 SimulationNov 4, 2025The SPHEREx Satellite MissionOct 30, 2025Galaxy Luminosity Function of the Coma Cluster from Deep $u'-g'-r'$ Wendelstein Imaging DataOct 30, 2025Accretion rates of stellar-mass compact objects embedded in AGN discsOct 29, 2025Extreme equivalent width-selected low-mass starbursts at $z=4-9$: insights into their role in cosmic reionizationOct 28, 2025PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-domain Field IIIOct 27, 2025Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44Oct 20, 2025Resolving the dusty star-forming galaxy GN20 at z=4.055 with NOEMA and JWST: A similar distribution of stars, gas and dust despite distinct apparent profiles