TY - GEN A1 - Gholami, Masoud A1 - Schintke, Florian A1 - Schütt, Thorsten A1 - Reinefeld, Alexander T1 - Modeling Checkpoint Schedules for Concurrent HPC Applications T2 - CoSaS 2018 International Symposium on Computational Science at Scale Y1 - 2018 ER - TY - GEN A1 - Dreßler, Sebastian A1 - Steinke, Thomas T1 - Automated Analysis of Complex Data Objects T2 - 28th International Supercomputing Conference, ISC 2013, Leipzig, Germany, June 16-20, 2013 Y1 - 2013 N1 - Posterbeitrag ER - TY - GEN A1 - Scheffler, Daniel A1 - Sips, Mike A1 - Behling, Robert A1 - Dransch, Doris A1 - Eggert, Daniel A1 - Fajerski, Jan A1 - Freytag, Johann-Christoph A1 - Griffiths, Patrick A1 - Hollstein, André A1 - Hostert, Patrick A1 - Köthur, Patrick A1 - Peters, Mathias A1 - Pflugmacher, Dirk A1 - Rabe, Andreas A1 - Reinefeld, Alexander A1 - Schintke, Florian A1 - Segel, Karl T1 - GeoMultiSens – Scalable Multisensoral Analysis of Satellite Remote Sensing Data T2 - ESA Living Planet Symposium, EO Open Science Posters Y1 - 2016 ER - TY - GEN A1 - Ragyanszki, Anita A1 - Ji, Hongchen A1 - Fournier, Rene T1 - Understanding the Origins of Life - A Machine learning approach to estimate reaction mechanisms of biotic precursors T2 - Perspectives and challenges of future HPC installations for atomistic and molecular simulations N2 - Life as we know it is the result of billions of years of evolution; yet, understanding how the very first organisms came into existence is a challenge that has yet to be solved. One theory states that components of the first biotic molecules may not have formed on Earth. Rather, they may have initially formed in the interstellar medium (ISM) and been transported to Earth, as supported by recorded instances of organic molecules detected in space. The ISM, with its low temperatures and specific collision processes, allows for molecular stability and the formation of biotic precursors that would otherwise be unlikely in Earth's prebiotic conditions. Understanding how these molecules formed in the ISM may be the key to determining how life began. The goal of this research is to develop a new model for solving astrobiophysical problems by studying the formation mechanisms of biomolecules found in the ISM. Although such pathways have been studied individually, there has not yet been a comprehensive method to understand all the formation reactions that can occur in ISM. Several quantum chemical and numerical methods are available for finding transition states (TS) and energy barriers (E) of chemical reactions but are time-consuming and can hardly be applied to systems with more than a few atoms. Our main interest is to develop a a machine learning approach to approximate TS, and E, requiring as input only estimates of geometry and energies of reactants and products. Using a complete dataset 300 reaction features are computed, and an estimate of E is obtained by fitting a Kernel Ridge Regression (KRR) model with Laplacian kernel, and a fully connected Artificial Neural Network (ANN) to estimate reaction energy barriers. Y1 - 2024 ER - TY - GEN A1 - Ragyanszki, Anita A1 - Ji, Hongchen A1 - Fournier, Rene T1 - Understanding the Origins of Life – A Machine learning approach to estimate reaction mechanisms of biotic precursors T2 - SIMPLAIX N2 - Understanding the Origins of Life - A Machine learning approach to estimate reaction mechanisms of biotic precursors. Life as we know it is the result of billions of years of evolution; however, understanding how the very first organisms came into existence is a challenge that has yet to be solved. One theory states that components of these molecules may have formed in the interstellar medium (ISM) and been transported to Earth. The ISM, with its specific conditions, allows for molecular stability and the formation of biotic precursors that would otherwise be unlikely in Earth's prebiotic conditions. Understanding how these molecules formed in the ISM may be the key to determining how life began. The goal of this research is to develop a model for solving astrobiophysical problems by studying the formation mechanisms of biomolecules found in the ISM. Although such pathways have been studied individually, there has not yet been a comprehensive method to understand the complete reactions mechanisms. Several QM methods are available for finding transition states (TS) and energy barriers (E) of chemical reactions but are time-consuming and can hardly be applied to more complex systems. Our interest is to develop a machine learning approach to approximate TS, and E, requiring as input only estimates of geometry and energies of reactants and products. Y1 - 2024 ER - TY - GEN A1 - Kharma, Sami A1 - Wies, Tobias A1 - Schintke, Florian T1 - Comprehensive Plugin-Based Monitoring of Nexflow Workflow Executions T2 - SCA/HPC Asia 2026 Y1 - 2026 UR - https://www.sc-asia.org/2026/data/poster/post140.pdf ER -