Instrumentation & methods
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- Tailoring Infra-Red Filters for Global Mapping of Enceladus' Thermal Environment
- OCCAMS: A Multi-Task Learning-Based Investigation of the CMB Power Spectra
- TEMPEST - A modular Python-based thermophysical model for rough, irregularly-shaped airless bodies
- On the Proper 3D Modeling of Orbits in Wide Binary Gravity Tests
- Measuring Precipitable Water Vapor through Dual-Band GPS at Rubin Observatory
- posterior-landscape: morphological feature finding in two-dimensional probability densities
- Model-Based Retrieval of Four Years of JWST/NIRCam Wavefronts
- Temporal regularization of petal modes in SCAO systems: The Soft-Limiter approach
- Beyond χ2: Ensemble null tests for reliable scientific discovery
- Seven Years of TESS Precovery Observations of the Dwarf-planet Candidate 2026 ED138
- Characterization of the CSST Survey Camera CCDs: I. basic electro-optical performance
- Addressing Exoplanetary Degeneracies Through Geometry: Application to Asynchronously Rotating Systems
- FARSim: a fast RF-chain-aware trigger-screening surrogate for radio detection of ultra-high-energy cosmic rays
- Identifying narrow-band mutual coupling resonances in SKA-low stations using frequency-independent current basis functions
- Benchmarking Quantum Neural Networks Developed for MBHB Coalescence in the Context of LISA Space Mission
- Preparation of a celestial field for precise VLBI observations of the JUICE spacecraft: a test case of the Venus flyby
- Sequince: a modular sequential Monte Carlo toolkit
- Robust statistical significance for Gravitational Wave inference
- The Radio Neutrino Observatory in Greenland (RNO-G) - System Design and Instrumentation
- Search for Cosmic Rays in GRANDProto300
- Towards an Astronomical Use of New-Generation Geodetic Observations
- Optical clock network tracks tidal variations of the gravity potential
- The Pointing Error Due To Laser Propagation in Space Plasma for TianQin Gravitational Wave Detection
- Efficient GLS map-making and assessment of 1/f noise impact for future CMB satellite missions
- Tabular Foundation Models Dramatically Outperform Bespoke Photometric Redshift Estimators