Instrumentation & methods
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- Data-driven characterisation of variable source light curves with multimodal representation learning
- Orientation-dependent sensitivity of the all-sky all-frequency gravitational-wave radiometer search to continuous-wave sources
- B-fields In STar-forming Region Observations (BISTRO): Dual-Wavelength Constraints on Size-Dependent Grain Alignment in Star-Forming Regions
- B-fields In STar-forming Region Observations (BISTRO): Technical Foundations for Quantitative 450/850 μm JCMT SCUBA-2/POL-2 Polarimetry
- How general relativity stacks up: Testing gravity by coherently combining gravitational-wave observations
- A Solar Optical Clock
- Impact of numerical stability in Bayesian noise wave calibration on global 21-cm experiments
- The Stellar "Snake"-V: the census within 3 kpc in the Solar Neighborhood
- A Unified HI Rotation Curve Database for 122 Dwarf and Irregular Galaxies
- An improvement to the spatial discretisation in the Astrophysical Weighted Particle Hydrodynamics method
- SIGNN++: Robust Graph Neural Star Identification on Earth
- Dual-Phase Flow Matching for Probabilistic Source Detection and Measurement in Astronomical Images
- KROME-X: a GPU-ready library for chemistry and microphysics in astrophysical simulations
- PIANISTpy: A JAX-based Python package for velocity-anisotropic astrophysical equilibrium models
- Systematic Uncertainties in Rocky Exoplanet Reflected Light from Incomplete Laboratory BRDF Measurements
- Prior volume effect inflates the gravitational-wave background in pulsar timing arrays
- Arepo-CD: Coupling Collisional N-Body Dynamics with Moving-Mesh Magnetohydrodynamics
- Noisy Pipelines I: An end-to-end pipeline to perform multivariate noise inference for LISA
- Solar System Surface Technosignatures: Searching for Signs of Artificial Design on Extraterrestrial Terrain
- Chana: A GPU-Accelerated Adaptive-Mesh Code for General Relativistic Magnetohydrodynamics with Multigroup M1 Neutrino Transport
- Community Lessons from builders of infrared multi-object spectrographs
- Revisiting the Unknown Unknowns in Transient Astrophysics with the SKA Telescopes
- The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres
- Phakoseismology: Asteroseismology of gravitationally microlensed stars
- Estimator Precision and Selection for Up-the-Ramp Sampling with a High-Read-Noise InGaAs Camera