Supporting data for “Positional and Flux anomalies caused by the granulation of wave dark matter”
收藏datahub.hku.hk2020-09-21 更新2025-01-15 收录
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https://datahub.hku.hk/articles/dataset/Supporting_data_for_Positional_and_Flux_anomalies_caused_by_the_granulation_of_wave_dark_matter_/12961763/1
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These are arrays containing the deflection fields for a galaxy lens, which allow us to carry out the calculation of the light magnification.The deflection fields are calculated by using the mass maps that describe the mass distribution of the gravitational lens.
本数据集包含描述星系透镜的弯曲场的数组,这些数组使我们能够进行光放大效应的计算。弯曲场是通过描述引力透镜质量分布的质量图计算得出。
提供机构:
HKU Data Repository



