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- Assessing the detectability of a realistic massive black hole binary population in LSST
- Dark Matter and MOND successes and degeneracies in reproducing SPARC rotation curves and weak lensing data
- El Ascua: An ultra-luminous, radio-loud, Compton-thick AGN at z∼ 3.8 hiding in plain sight revealed by MINERVA multi-band MIRI observations
- A Composite Rest-Frame UV Spectrum of Galaxies at 5.7 < z < 6.9: Ionization, Outflows, and Implications for Intergalactic Metal Enrichment
- Comprehensive Visible and Near-infrared Keck and Gemini Monitoring and Characterization of Interstellar Comet 3I/ATLAS during its Encounter with the Solar System
- A probabilistic approach to separate mergers and jellyfish galaxies: Application of morphological non-parametric indexes to the DESI Legacy Survey
- One-Million-Year-Old Nascent Eclipsing Binaries in the LMC
- A Population Synthesis Model for Odd Radio Circles Produced by Shock-Bubble Interactions
- Complete Multi-Band Structural Characterization for 10 Million Galaxies in the Hyper Suprime-Cam Wide Survey using Deep Learning
- Physics Informed Neural Network for Multi-dimensional Turbulent Self-gravitating Flows
- The Physics of the Cold and Warm Interstellar Medium Through Radio Recombination Lines
- Research of signs of star formation in three S0 galaxies - members of isolated pairs
- Magnetic Reconnection Modifies Cosmic-Ray Transport in the Interstellar Medium
- Spatial distribution of star formation in dwarf galaxies: Merger-driven and secular starburst
- Polarization Observations of NGC 315 with FAST
- Forward model of the Gaia DR3 selection function
- The Galactic rotation curve from the ALS III catalogue of OB Stars
- Star clusters at cosmic dawn I: the emergence of the initial cluster mass function
- Local Analogs of Little Red Dots: Clues to the X-ray Weakness
- Binary Dynamics and Mergers in a Stellar Disk and the Formation of Dusty Objects in the Galactic Center
- Differential and integral scaling laws of the mass density of molecular clouds
- Galaxy Luminosity Functions at z~7-10 from Four Years of JWST Observations
- SMMAN Studies of AGN Variability. I. Long-term Spectral Evolution and a Candidate ∼1000-day Quasi-periodic Modulation in 4C+72.28
- A neural-network model to find correlations in astrochemical space
- The ALMA REBELS Survey: The [C II] Luminosity Function of UV-Selected Galaxies at z∼7