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- The differences in the narrow-line region of nearby QSOs 1 and QSOs 2 – II. Signatures of kinetic feedback
- Investigating the star formation histories of galaxies from cosmic dawn to the Epoch of Reionization with the Santa Cruz SAM
- The Metal Content of Resolved Galaxies
- Synthetic Spectral Library of Optically Thick Atmospheres for Little Red Dots
- Effect of Local Environment on Ly α Line Profile in DESI/ODIN LAEs
- Galactic Tides and the Outer Density Profile of the Sculptor and Ursa Minor Dwarf Spheroidals
- JWST/NIRSpec Reveals Diverse Nuclear Environments in Dwarf Galaxies Hosting Active Galactic Nuclei
- Direct Pathway to the Early Supermassive Black Holes: A Red Super-Eddington Quasar in a Massive Starburst Host at z = 7.2
- The COSMOS-Web Lens Survey (COWLS) III: forecasts versus data
- The [Y/Mg] chemical clock and the stellar ages of solar-type stars in the solar neighbourhood
- Predicted state-to-state collisional rate coefficients from neural networks
- Bridging Theory and Observation: Synthetic Far-infrared Insights into Star Formation Efficiency
- Exploring Case B I: The Footprints of Hidden Radiation Fields in H I Balmer Decrements
- When dust growth takes over: the origin of dust in post-reionization galaxies
- A Single Line-Emitter Identified in an Unbiased Search with JWST/NIRSpec: Multi-Object Coronagraphy for Slitless Spectroscopy
- Galaxy Clustering Can Reveal Host-Galaxy Properties of Binary Black Hole Mergers
- Disk Structure May Determine AGN Variability and Explain the Accretion Disk Size Problem: No Broad Line Region Required
- ACORN I. Massive Black Hole Seeding and Tidal Disruption Events from Star Clusters in Cosmological Simulations
- Inflow-driven galaxy evolution - II: A hierarchy in the scaling relations of star-forming galaxies
- JWST CAPERS: Spectroscopic evaluation of very high redshift galaxy candidates
- Modeling CO Line Luminosity Using FIRE Simulations: I. Methodology and Validation of Molecular Gas and CO Abundance
- Discovery of the Slowest Radio Pulsar in the Small Magellanic Cloud
- Too many or too bright? Status and perspectives in the study of the UV Luminosity Function at z>10
- EWOCS-XI: Anisotropic expansion and shear in the cluster Westerlund 1. A 2D kinematic analysis with Gaia DR3
- Binding Energies of Astrophysically Relevant Molecules on CO2 Clusters: Benchmarking and the Donor-Acceptor Origin of Surface-Dependent Binding