How to use the autogalaxy.util.cosmology_util.arcsec_per_kpc_from function in autogalaxy
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Jammy2211 / PyAutoLens / autolens / lens / ray_tracing.py View on Github 
def arcsec_per_kpc_proper_of_plane(self, i):
return cosmology_util.arcsec_per_kpc_from(
redshift=self.plane_redshifts[i], cosmology=self.cosmology
)autogalaxy
Open-Source Multi Wavelength Galaxy Structure & Morphology
Package Health Score
72 / 100Popular autogalaxy functions
- autogalaxy.galaxy.fit_galaxy.FitGalaxy
- autogalaxy.galaxy.masked_galaxy_data.MaskedGalaxyDataset
- autogalaxy.GalaxyModel
- autogalaxy.pipeline.phase.dataset.analysis
- autogalaxy.plane.plane.Plane
- autogalaxy.plot
- autogalaxy.plot.FitInterferometer.chi_squared_map_vs_uv_distances
- autogalaxy.plot.FitInterferometer.normalized_residual_map_vs_uv_distances
- autogalaxy.plot.FitInterferometer.residual_map_vs_uv_distances
- autogalaxy.plot.inversion_plots
- autogalaxy.plot.inversion_plots.individuals
- autogalaxy.plot.inversion_plots.reconstruction
- autogalaxy.plot.lensing_plotters
- autogalaxy.plot.lensing_plotters.Include
- autogalaxy.plot.lensing_plotters.set_include_and_plotter
- autogalaxy.plot.Plane.plane_image
- autogalaxy.plot.plane_plots.plane_image
- autogalaxy.util.cosmology_util
- autogalaxy.util.cosmology_util.arcsec_per_kpc_from
- autogalaxy.util.cosmology_util.scaling_factor_between_redshifts_from