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- J-PAS: Exploring the connection between local environment and the triggering of bursty star formation in Extreme Emission Line Galaxies
- Kinematic analysis of the TNG50 Milky Way and Andromeda analogues
- An Empirical Temperature Relation for Chemical Abundances in AGN
- Two Fast Radio Burst Candidates Detected in the RATAN-600 Blind Survey
- See you again: an 80∘ NGC~5466 stellar stream and its constraints on the Galactic dark halo mass
- The Stellar-Mass Dependence of Feedback-Driven Outflows in DESI DR1 Star-Forming Galaxies
- An all-sky catalogue of Be transition stars from WISE and Gaia
- Chemical abundances of a Galactic Centre ejecta discovered in DESI
- Harmonic Angular Mapping Method for Binary Microlensing Grid Search
- Sub-sonic compressible magnetohydrodynamic turbulence I. Alfvénic and fast-magnetosonic injection, amplitude dependence, and compressibility effects
- Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals
- First Light and Reionization Epoch Simulations (FLARES) XXII: UV-dust spatial offsets at the Epoch of Reionisation
- Inside the cocoon: A comprehensive explanation of the spectra of little red dots
- Simulating winds in the Galactic centre. II. Observational biases on HI clouds and a multi-wavelength comparison
- An Unusually Clumpy Ultra-Diffuse Galaxy in the Coma Cluster: A Missing Link for Globular Cluster Formation?
- Physically Motivated Stellar Populations for Galaxies at Cosmic Dawn with a Temperature-Dependent IMF
- Dynamically defined bulges reveal that early-type galaxies with compact bulges host more massive black holes
- Witnessing pre-processing at intermediate redshift: observational evidence of infalling groups onto a merging galaxy cluster
- Introducing Aurora: A New Black Hole Seeding Model With Explicit Environmental Coupling
- Tracking the evolution of sub-Neptunes. I. Gyrochronology of planet hosting stars
- EMU/GAMA: Understanding the link between dust geometry and star formation rate in galaxies
- Boosted Physics-Informed Neural Networks for Solving Homogeneous and Non-Homogeneous Lane-Emden Type Equations
- Modeling CO Line Luminosity with FIRE simulations: II. Comparison With Observations, CO Luminosity Functions and Redshift Evolution
- The L1157 filament as traced in HNCO by the LMT
- Euclid Quick Data Release (Q1). Mass-to-light ratio of elliptical galaxies: constraints from strong lensing