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- Isophotal signatures of the brightest cluster galaxy - intracluster light transition
- A full chemical network treatment of supermassive black hole seed formation from dark matter annihilation or decay
- Lyα in Compact Broad-Line Emitters, Including Little Red Dots, Is More Closely Linked to the Host Galaxy than to the Broad-Line Nucleus
- Tiny Galaxies, Mighty Nitrogen: Linking Chemical Anomalies to Compact Galaxies at High Redshift using JWST/JADES
- Surface Nitrogen enrichment from the LMC to the Early Universe: the roles of rotation, overshooting and mass loss
- Jets and winds from the most powerful compact object in NGC 5408
- Gaia's dark partners: A new signature of dissipative dark matter
- How bursty star formation shapes spectral diversity at high redshifts: breaking degeneracies in early galaxy formation
- Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model
- Episodic Star Formation - II. The Origin of the Fundamental Metallicity Relation
- Chemical and dynamical evolution of prestellar cores, the dawn of star and planet formation
- Episodic Protostellar Outflows: A Proper Motion Study in Serpens South
- VLITE Observations of the Hubble Ultra Deep Field
- A Physics Informed Neural Network Approach to Decipher Environmental Confinement of Molecular Clouds in the Third Galactic Quadrant
- Stellar wind variability in OB stars and its effect on mass-loss determinations
- A Cepheid-based Distance to the Type 1 Seyfert NGC 3783
- Statistical Modeling of Foreground Galactic Cirrus for Diffuse Halo Light Measurement
- Molecular gas in the disks and tails of ram pressure stripped Coma galaxies
- Lyman-alpha haloes in the aftermath of reionisation
- A MIGHTEE robust measurement of the star formation rate-radio correlation
- The Milky Way's Missing In-Situ Halo
- The Quasar Main Sequence of Highly Accreting NLSy1 Galaxies
- GALACTIC CENTERS AS TRACERS OF GALAXY EVOLUTION: Zooming from galaxy large-scale properties into their central massive black holes
- What can strong lensing recover in edge-on disc galaxies? A mock study based on TNG50 simulations
- Decomposition of disk and jet optical emission: Case of PKS~1510-089 and PKS~0736+017