Instrumentation & methods
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- Empirical verification of principal mode orthogonality and relative phase calibration in photonic lanterns
- An agentic framework for gravitational-wave counterpart association in the multi-messenger era
- VLTI/MATISSE observations of the hot dust around β Pictoris Observing faint objects with MATISSE
- Mining the time axis with TRON - III. Discovery of a nulling pulsar towards the SMC with MeerKAT
- A cosmic-ray database update: CRDB v4.2
- nufftcf: Fast Auto- and Cross-Correlation Function Estimation for Irregularly-Sampled Time Series via the Non-Uniform FFT
- Multimessenger Spectroscopy
- NEO-BENCH: A New Multi-Source Benchmark for Generalizable Astronomical Streak Detection
- Calibration of CNEOS Fireball Velocities and the Robustness of Nominally Hyperbolic Events
- Chromatic Anisoplanatism in Adaptive Optics: A detailed comparison of theory with numerical simulations
- PySeshat: A Validated Python Pipeline for Binary-Star Orbit Determination and Al-Wardat Stellar Atmosphere Modeling
- Generating radio continuum survey maps of arbitrary size with latent diffusion models
- Mechanisms of Electrostatic Charge Formation and Retention in Lunar Regolith
- DustRover: A Python Package for Modelling Dust Extinction Curves (Phase I)
- PERRY: A Human-in-the-Loop GUI for Precision Alignment of MUSE Data
- Recovering Weak Signals with Normalizing Flows
- Optical Colors as Compressed Spectral Information for Trans-Neptunian Objects
- High-Power AM-CW Lunar Laser Ranging as a μHz SGWB Detector
- Alternative neural-network follow-up for all-sky FrequencyHough in continuous gravitational-wave searches
- Self-supervised reconstruction of transients in data from space-borne gravitational-wave detectors
- POSTELLAR: Posterior Stellar Spectrum Sampling - An Alternative to Approximate Stellar Spectra for Exoplanetary Analysis
- Rotational broadening of exoplanet spectra in arbitrarily oriented systems: Application to reflected light
- Unresolved Binary Systems in the Rubin Era I: An Autoencoder Framework for Binary Identification Applied to 47 Tucanae
- Fast Lensing And Sub-minute High-accuracy photometry (FLASH) with JWST: Pipeline and Primordial Black Hole Microlensing Constraints from M31
- The information content of optical intensity interferometry