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  1. Free, publicly-accessible full text available December 1, 2026
  2. Abstract Increasing the number of organ donations after circulatory death (DCD) has been identified as one of the most important ways of addressing the ongoing organ shortage. While recent technological advances in organ transplantation have increased their success rate, a substantial challenge in increasing the number of DCD donations resides in the uncertainty regarding the timing of cardiac death after terminal extubation, impacting the risk of prolonged ischemic organ injury, and negatively affecting post-transplant outcomes. In this study, we trained and externally validated an ODE-RNN model, which combines recurrent neural network with neural ordinary equations and excels in processing irregularly-sampled time series data. The model is designed to predict time-to-death following terminal extubation in the intensive care unit (ICU) using the history of clinical observations. Our model was trained on a cohort of 3,238 patients from Yale New Haven Hospital, and validated on an external cohort of 1,908 patients from six hospitals across Connecticut. The model achieved accuracies of$$95.3~\pm ~1.0\%$$and$$95.4~\pm ~0.7\%$$for predicting whether death would occur in the first 30 and 60 minutes, respectively, with a calibration error of$$0.024~\pm ~0.009$$. Heart rate, respiratory rate, mean arterial blood pressure (MAP), oxygen saturation (SpO2), and Glasgow Coma Scale (GCS) scores were identified as the most important predictors. Surpassing existing clinical scores, our model sets the stage for reduced organ acquisition costs and improved post-transplant outcomes. 
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    Free, publicly-accessible full text available December 1, 2026
  3. Free, publicly-accessible full text available December 31, 2026
  4. Free, publicly-accessible full text available November 1, 2026
  5. Operators of web archives have two options for how to crawl pages from the web. Browser-based dynamic crawlers capture all of the resources on every page, but incur high compute overheads. Static browserless crawlers are more lightweight, but miss page resources which are fetched only when scripts are executed. In this paper, we make the case that a web archive does not have to make a binary choice between dynamic or static crawling. Instead, by using a browser for a carefully chosen small subset of crawls, an archive can significantly improve its ability to serve statically crawled pages with high fidelity. First, we show how to reuse crawled resources, both across pages and across multiple crawls of the same page over time. Second, by leveraging a dynamic crawl of a page, we show that subsequent static crawls of the page can be augmented to fetch resources without executing the scripts which request them. We estimate that, as long as 8.9% of page crawls use a browser, an archive can serve roughly 99% of the remaining statically crawled pages without any loss in fidelity, up from 55% without our techniques. 
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    Free, publicly-accessible full text available October 28, 2026
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  7. Free, publicly-accessible full text available October 26, 2026
  8. Abstract AstroSage-Llama-3.1-8B is a domain-specialized natural-language AI assistant tailored for research in astronomy, astrophysics, cosmology, and astronomical instrumentation. Trained on the complete collection of astronomy-related arXiv papers from 2007 to 2024 along with millions of synthetically-generated question-answer pairs and other astronomical literature, AstroSage-Llama-3.1-8B demonstrates remarkable proficiency on a wide range of questions. AstroSage-Llama-3.1-8B scores 80.9% on the AstroMLab-1 benchmark, greatly outperforming all models—proprietary and open-weight—in the 8-billion parameter class, and performing on par with GPT-4o. This achievement demonstrates the potential of domain specialization in AI, suggesting that focused training can yield capabilities exceeding those of much larger, general-purpose models. AstroSage-Llama-3.1-8B is freely available, enabling widespread access to advanced AI capabilities for astronomical education and research. 
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    Free, publicly-accessible full text available December 1, 2026
  9. Abstract Laser ablation is a process that bears both fundamental physics interest and has wide industrial applications. For decades, the lack of probes on the relevant time and length scales has prevented access to the highly nonequilibrium phase decomposition processes triggered by laser excitation. In this study, a close integration of time-resolved probing by intense femtosecond X-ray pulses with large-scale atomistic modeling has yielded unique insights into the ablation dynamics of thin gold films irradiated by femtosecond laser pulses. The emergence and growth of nanoscale density heterogeneities in the expanding ablation plume, predicted in the simulations, are mapped to the rapid evolution of distinct small angle diffraction features. This mapping enables identification of the characteristic signatures of different phase decomposition processes occurring simultaneously in the plume, which are driven by photomechanical and thermodynamic driving forces. Beyond the specific insights into the ablation phenomenon, this study demonstrates the power of joint X-ray probing and atomistic modeling of material dynamics under extreme conditions of thermal and mechanical nonequilibrium. 
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    Free, publicly-accessible full text available December 1, 2026
  10. Free, publicly-accessible full text available October 31, 2026