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- Connecting galaxy structure, quenching, and halo environments during cosmic noon
- Dynamical response of a protoplanetary disk to an FU Ori-type outburst
- IMF-aware N-body forward modelling of membership selection functions for young open clusters
- The dawn of the first galaxies
- Galactic Outflows and Star-Formation Quenching: A JWST Perspective
- Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data
- Supermassive Black Hole Winds in X-rays -- SUBWAYS. VI. Interplay between the soft X-ray excess and ultra-fast outflows
- The Star Formation Histories of Different Components of M31's Halo from Photometric Estimates of Fe and α Abundances
- The Impact of an AGN on PAH Spectral Features in Galaxy Evolution Simulations: Continuum Dilution and Excitation of PAHs
- Clumpy Outflows from Super-Eddington Accreting Black Holes. II. Conditions for Clump Formation
- Galactic warps constrain equivalence-principle violation in the dark sector
- Forecasting the Resolvability of Stellar Velocity Dispersions in Ultra-faint Dwarf Galaxies
- Newly Identified Planetary Nebula Candidates in M31 using Deep-Learning Search of Hubble Space Telescope Images
- Statistical Strong Lensing V. Inference with Microlensed Quasars
- Spiraling into the `snail' cluster MCXC J0157.4-0550
- Molecular and Atomic Gas Associated with the Gamma Ray Supernova Remnant RCW 103
- Morphological Bias: How Ellipticals and Spirals Trace the Cosmic Web Differently
- Modeling Multi-band Active Galactic Nuclei Lightcurves Using an Self-supervised Attentive Neural Process Network
- A DECADE of Giants: A catalog of 42,000 optically identified galaxy clusters from 13,000 deg2 of the sky
- The evolution of 3C 306 in the galaxy cluster RXCJ1454.4+1622: linking spectral ageing, ICM conditions, and jet dynamics through MHD simulations
- Can Blue UV-Bright Galaxies Drive Reionization at Cosmic Dawn? An MUV=−19.6 Galaxy with fesc≈0.85 at z=9.244
- Beyond the dust: JWST reveals extinction and ice content in local (U)LIRGs
- Calibration of the Next Generation Palomar Spectrograph as a Stellar Speedometer
- Revisiting the Mass and Scale Dependence of the "Lensing is Low" Effect with DECADE
- A precessing AGN with S-shaped morphology discovered in MALS