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Cuándo Usar el Explorador 3D de Lente Gravitacional Fuerte - Mejores Sesiones y Límites


Abre el Explorador 3D de Lente Gravitacional Fuerte cuando quieras ver cómo la alineación entre una fuente de fondo y una lente en primer plano convierte un solo objeto en varias imágenes o arcos largos - no para consultar el modelo de masa exacto medido de un objeto específico.


Un patrón guiado por la alineación, no una sola imagen fija

Una sesión empieza eligiendo el caso de la Cruz de Einstein para ver 4 imágenes puntuales alrededor de una galaxia en primer plano con corrimiento al rojo 0,0394 lentificando un cuásar con corrimiento al rojo 1,695, luego cambiando al caso Abell 2218 para ver decenas de arcos de galaxias de fondo con corrimientos al rojo de hasta unos 2,5 - arrastrar el control deslizante de alineación en cualquier caso desvanece las imágenes adicionales o acorta los arcos.


Sesiones que este explorador no cubre

Sesiones que esta página no cubre son consultar un modelo de lente resuelto numéricamente para la distribución de masa exacta de cualquier objeto, o el caso simétrico especial en que la alineación es exacta y las imágenes se fusionan en un solo anillo completo - ese caso está en el Explorador 3D del Anillo de Einstein. Recorre los controles en la guía paso a paso.

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