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- Focal plane modal estimation of high-order wavefront drifts on coronagraphic testbeds
- Phase-resolved X-ray spectroscopy of the Vela pulsar with NICER observations
- Search for Eccentric Neutron Star-Black Hole Binaries in Advanced LIGO's Fourth Observing Run using Effective-One-Body Waveforms
- The Carousel Lens III: Joint lens convergence and source kinematic modeling
- Probabilistic Stellar Mass and Radius Estimation with Bayesian Hierarchical Stacking
- Simulating and Characterizing Non-Gaussian Small-Scale Polarized Emission
- Machine learning applications in the heliosphere
- Validating an X-ray-based method for identifying Fermi blazars
- Considering Numerical Relativity Surrogate Models for AGN Channel Merger Dynamics
- The MARTINI platform II. Tracing r-process nucleosynthesis in neutron star mergers with long-lived remnants
- No Significant Excess in Typical Variability in CLAS+ Changing-Look AGN Candidates in Rubin DP2
- Combining Multiple Incomplete Astronomical Surveys to Estimate Galaxy Flux Distributions
- Core-collapse universality for inelastic self-interacting dark matter halos
- Early Dark Energy Crowds Out Interacting Dark Energy
- Probing Cosmology with Diffusion Models: Memorization, Generalization, and Parameter Estimation
- Simulation-Informed Dust Masses in Typical 6<z<14 JWST Galaxies
- Searching for Circumplanetary Dust in the Cavity of the AB Aurigae Disk with ALMA
- Primordial Gravitational Waves in Loop Quantum Cosmology: Regularization Ambiguities and Initial State Dependence
- Revisiting Sub-Neptune Population Synthesis: The Role of Core Luminosity in Boil-off, Photoevaporation, and the Radius Distribution
- The Redshift-Space Cluster-Galaxy Cross-Correlation as a Probe of Gravity on Cosmic Scales
- Ejected and Rejected: Strong Scatterings in Dense Star Clusters
- Not so dead after all: young stars in the massive S0 NGC 3115
- A double debris disc around a white dwarf sculpted by two planetary bodies
- Extra! Extra! X-ray Emission!: X-rays in Romulus25, Part II - Physical Drivers of X-ray Emission in the CGM
- NORI: a GPU-accelerated code for simulating self-gravitating and self-interacting dark matter