1. National Science Foundation's Very Large Array radio telescope in New Mexico and the Plateau de Bure Interferometer in France.
   专家们说，这些发现将会使科学家们对星系的诞生有个更加清晰的认识。
2. The detection and reconstruction of wavefront by Lateral Shear Interferometer (LSI) and Hartmann Wavefront Sensor (HWS) have been deduced analogically and simulated numerically.
   对横向剪切干涉仪和哈特曼波前传感器的波前探测和复原进行了类比推导和仿真计算。
3. The light gathering power of the interferometer, the etendue in the object space and the conditions of matching one to the another are given.
   给出了干涉仪聚光本领、物空间聚光本领及其二者的匹配条件;

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