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- GetGaia 2.0: automatic membership and systemic motions of stellar systems with Gaia
- CosmicGrain: An On-the-fly Dust Physics Module
- Formamide formation on forsterite and Mg(OH)2·H2O
- A Machine Learning Approach to Coupling Photoionization & Multi-Frequency Radiation Hydrodynamics
- Detection of Differential Chromatic Refraction with LSST Camera data
- Eddies that ride the flow: a model of turbulence with Richardson dispersion and anomalous dissipation
- Feedback-Driven Star Formation and YSO Distribution around H II Regions Sh2-140 and Sh2-145
- On the importance of medium-resolution continuum spectroscopy for JWST's extragalactic legacy
- The ALPINE-CRISTAL-JWST Survey: The Tully-Fisher Relation at z = 4−6
- The HST-Hyperion Survey: X-ray AGN Enhancement in the Hyperion Proto-supercluster
- DOWSING, Dust Observations With SCUBA-2 In Nearby Galaxies: I. Dust in M81
- A multi-epoch VLBI study of compact symmetric objects as contaminants in the search for milli-lenses
- AGN Archaeology: A Systematic Search for Fading AGN in MaNGA
- Why a Multi-Cycle Treasury Program is Essential to Maximize JWST's Scientific Contributions to Galaxy Formation
- The obscured nucleus of NGC3256 S. I. Anisotropic AGN near-IR radiation field traced by CO v=1-0 with JWST/NIRSpec
- Probing Dark Matter-Electron Scattering with the Central Molecular Zone
- Black Hole Seeds and Little Red Dots: Connecting Formation and Growth with a JWST Multi-Cycle Treasury Program
- SHARP(ening the) view of unresolved globular clusters in ultra diffuse galaxies
- Unveiling the Origins of Local Group Galaxies with ELT-SHARP: An Overview of Science Cases
- A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec ∼3-15
- ReveaLLAGN 3: Revealing the Infrared Spectral Energy Distributions of Low Luminosity AGN
- Magnetic Properties of Galactic Molecular Clouds
- Euclid Quick Data Release (Q1). Refining the strong lens sample with Space Warps crowd-sourced science
- The formation and evolution of Wolf-Rayet stars with temperature-dependent winds
- Investigating the initial conditions of globular clusters via N-body simulations: I. half-mass radius and stellar density