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[ascl:1901.008] SEDobs: Observational spectral energy distribution simulation

SEDobs uses state-of-the-art theoretical galaxy SEDs (spectral energy distributions) to create simulated observations of distant galaxies. It used BC03 and M05 theoretical models and allows the user to configure the simulated observation that are needed. For a given simulated galaxy, the user is able to simulate multi-spectral and multi-photometric observations.

Code site:
https://astrom-tom.github.io/SEDobs/build/html/index.html https://test.pypi.org/project/sedobs/
Bibcode:
2019ascl.soft01008T

Views: 561

ascl:1901.008
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