Instrumentation & methods
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- A Full-Sky SPHEREx Map of Integrated 3.3 and 3.4 μm PAH Emission
- ALMA - CTAO synergies
- On-sky commissioning and technical performance of Proto-NUX at Pic du Midi
- Detecting atmospheres in the presence of stellar contamination: an empirically calibrated framework applied to four JWST/NIRSpec PRISM transits of TRAPPIST-1c
- Scaling RIFT 1: Extending RIFT to third-generation gravitational-wave analyses
- Gravitational-Wave Inference For Noise PSD Jumps Across Data Gaps
- First laboratory demonstration of iEFC for high-contrast imaging at small angular separation on ELT scales
- Detecting Extragalactic Exoplanets With Fast Radio Burst Nanolensing
- LUMA: A CNN for Strong Gravitational Lens Searches in Astronomical Imaging
- Morphological Identification of Dynamical Regimes in MHD Turbulence with ScaleAware-JEPA
- A Bayesian Inference Framework for Binary Lens Events Fully Incorporating Higher-Order Effects
- ECLIPSE-X: Plate-Scale Calibration as the Binding Constraint on Relativistic Astrometry with Spacecraft Navigation
- Refactoring the SIXTE simulator: Towards a more modular code base
- HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
- On-Orbit Calibration of Danuri/PolCam. II. Image Artifact Correction
- Identifying Planetary Nebulae Candidates from IPHAS and VPHAS+ Surveys via YOLO Deep Learning Models
- Multi Kernel Gaussian Process Guiding: Predictive Correction for Mounts with Several Gear Stages
- Diffusion Models for Polarimetric Reconstruction of Circumstellar Environments in Correlated Speckle Noise
- Properties of Circumfacular Regions derived from Hα and Ca II K synoptic observations of the Sun
- Comparing Active Anomaly Detection Frameworks: From Light Curves to Images
- First Detection of the Doppler Shift of X-ray Photons Due to a Telescope's Orbital Motion
- Divergence-free magnetohydrodynamics on a moving mesh
- Improved Modeling for Moving Sources of Radio Frequency Interference and Impact on Flagging Strategies
- GameDev: GPU-accelerated model for dust evolution
- SIFARI: Self-Supervised Interferometric Fitting for Astronomical Radio Imaging