(Universidad de Surrey, Reino Unido): Sus intereses de investigaci\u00f3n se centran en revelar las historias evolutivas y el contenido de materia oscura de galaxias cercanas, mediante estudios forenses de las propiedades qu\u00edmicas y din\u00e1micas de las estrellas que las componen. Su especialidad es la construcci\u00f3n de modelos din\u00e1micos en equilibrio que conectan los movimientos estelares con la materia oscura, as\u00ed como el etiquetado din\u00e1mico que clasifica las estrellas seg\u00fan sus \u00f3rbitas. Tambi\u00e9n es experta en la aplicaci\u00f3n de Aprendizaje Autom\u00e1tico Bayesiano, por ejemplo, en la determinaci\u00f3n de las edades de tres millones de estrellas. Ha desarrollado un m\u00e9todo acelerado de Monte Carlo Hamiltoniano para muestrear funciones de distribuci\u00f3n de probabilidad, el cual se basa adicionalmente en teor\u00eda din\u00e1mica. Por \u00faltimo, es experta en la clasificaci\u00f3n de poblaciones estelares a partir de sus patrones de abundancia qu\u00edmica y en relacionar estos con sus historias evolutivas.<\/p>\n\n\n\n
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