Supporting data for “Positional and Flux anomalies caused by the granulation of wave dark matter”
datasetposted on 21.09.2020 by Alfred Amruth
Datasets usually provide raw data for analysis. This raw data often comes in spreadsheet form, but can be any collection of data, on which analysis can be performed.
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.