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- Bridging integrated-light and resolved-star studies of Local Group dwarf spheroidals
- Learning cosmic web environments with diffusion models
- Photometric redshifts for active galactic nuclei with LePHARE for the Vera C. Rubin Observatory
- The Fornax Cluster VLT Spectroscopic Survey
- On the Evolution of Circumstellar Disks Modified by the Presence of a Binary
- Effects of Synchrotron Self-Absorption on Polarization Diagnostics of MHD Turbulence
- Emission line stacking on cosmological scales: equivalence to two-point statistics and modelling of the observational effects
- Catastrophe Structure and Stability of Axion Stars
- Late Epoch Infrared Spectroscopy and Two-Component 3D Photoionization Modeling of Classical Nova V5668 Sgr
- Rest-frame Ultraviolet Variability of Quasars in the Cosmic Himalayas Overdensity
- A Kinematic Measurement of the Effective Viscosity of the Intracluster Medium: The Cold Front of A3667 Seen by XRISM
- S301 and friends: Measuring the spin of Sgr A*
- Resolving Galactic and Cluster Dynamics Without Dark Matter: Tsallis Entropy as the Unique Foundation of Emergent Gravity
- ALMA visits the QSO MUSEUM: Connecting molecular gas and the cool circumgalactic medium around 37 z∼3 quasars
- Detection of star formation in a near-pristine pocket of the Universe
- The descendants of z ≳ 10 JWST galaxies in the COLIBRE simulations
- How cluster pressure profiles scale: Mass, redshift, and intrinsic scatter
- Constraining the shape of dark matter haloes using only starlight
- The SIRMOS mission concept: a space-based near-IR spectroscopic survey of 100 million galaxies in the Euclid Wide Survey footprint
- Exploring the UV Fe III Emission along the Quasar Main Sequence
- Initial Conditions of Magnetized AGN Accretion Disks from Cloud Capture and Disruption
- Recently launched AGN-driven outflow in a lensed quiescent galaxy at Cosmic Noon
- How Steep is your Dust? Direct Measurements of Nebular Attenuation Curves at Cosmic Noon with JWST
- The Hosts and Mass Distribution Function of the Most Massive Black Holes: Implications for the nHz Gravitational Wave Background
- SN Ares: A Strongly Lensed Type IIb Supernova at z=1.276 with a Predicted 70-Year Time Delay