Showing 1–20 of 22 results
/ Date/ Name
Sep 26, 2024Confidence intervals uncovered: Are we ready for real-world medical imaging AI?May 7, 2025False Promises in Medical Imaging AI? Assessing Validity of Outperformance ClaimsMar 22, 2023Deployment of Image Analysis Algorithms under Prevalence ShiftsJun 3, 2022Metrics reloaded: Recommendations for image analysis validationJan 23, 2026Performance uncertainty in medical image analysis: a large-scale investigation of confidence intervalsNov 17, 2022Sources of performance variability in deep learning-based polyp detectionApr 12, 2021Common Limitations of Image Processing Metrics: A Picture StoryJun 6, 2025Challenging Vision-Language Models with Surgical Data: A New Dataset and Broad Benchmarking StudyDec 3, 20256 Fingers, 1 Kidney: Natural Adversarial Medical Images Reveal Critical Weaknesses of Vision-Language ModelsNov 5, 2025Current validation practice undermines surgical AI developmentJul 6, 2023Discovering new B[e] supergiants and candidate Luminous Blue Variables in nearby galaxiesFeb 3, 2023Understanding metric-related pitfalls in image analysis validationSep 13, 2022Using machine learning to investigate the populations of dusty evolved stars in various metallicitiesSep 18, 2025Sequential sample size calculations and learning curves safeguard the robust development of a clinical prediction model for individualsDec 19, 2025Medical Imaging AI Competitions Lack FairnessFeb 19, 2024Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicityApr 1, 2025A machine-learning photometric classifier for massive stars in nearby galaxies II. The catalogAug 9, 2023Introducing the ASSESS project: Episodic Mass Loss in Evolved Massive Stars -- Key to Understanding the Explosive Early UniverseMay 17, 2024Episodic mass loss in the very luminous red supergiant [W60] B90 in the Large Magellanic CloudOct 30, 2025Investigating episodic mass loss in evolved massive stars IV. Comprehensive analysis of dusty red supergiants in NGC 6822, IC 10, and WLM