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- Aperture-dependent [O III] profile variability: Clues to the nature of double-peaked narrow emission lines
- Spectroscopy-informed Deep Learning Searches for Photometric Little Red Dots in JWST Surveys
- Spacetime Evolution Induced by a Massive Cosmic String in Numerical Relativity
- Spectroscopic diagnostics of coronal fan loops using EIS/Hinode and AIA/SDO
- Orbital Architecture of Super-Earth-Cold-Jupiter Systems from Transit Duration Ratios
- Longitudinal-field particle acceleration in channels generated by strong electromagnetic waves in pair plasma
- Gravitational-Wave Microlensing as a Probe of Compact Object Population
- Tiny Quiet-Sun EUV Ejections Revealed by High-resolution Multiwavelength Observations
- Collective Characterization of Polar Crown Filament Eruptions
- Frequent Optical Flares in an M-type Detached Eclipsing Binary TIC 349005337
- The kinematic Kelvin-Helmholtz instability-driven dynamo: implications for merging compact objects
- Mock CSST NUV-NIR imaging of TNG50 galaxies with resolved stellar populations
- Polarimetry with the Giant Magellan Telescope: A Scientific Justification & Technical Requirements Document
- Photometric Study of a Distant SU UMa-type Dwarf Nova KSP-OT-201803a
- A Laplace-Transform Green's Function for Two-Zone Diffusion with Energy Losses: Application to the Geminga Pulsar Halo
- Unsupervised Neural Operators for Rotating Relativistic Stars: High-Fidelity Equation of State Inference and Pulsar Spin Evolution at Scale
- Insights on the mass composition of ultrahigh-energy cosmic rays from small-scale anisotropy with large-scale structure simulations
- How fast is the fastest-rotating O-type star in the Galaxy?
- Inferring Properties of Rotating Core-Collapse Supernovae with Gravitational-Wave Detector Networks
- Fast Graph-based Higher-Order Clustering Statistics on the GPU
- Precision Solar System Dynamics for Ultralight Dark Matter Search
- Probing IMF Variations in High-Redshift Early-Type Galaxies with SHARP
- A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon
- A new era for Dual AGN science with SHARP
- SHARP -- A spectrograph proposal to fully exploit ELT capabilities and look beyond JWST