Photometry¶
With spectra in hand we can produce photometry by combining the Sed object containing the (multidimensional) spectra with a FilterCollection defining the transmission curve of a set of filters.
Doing so produces a PhotometryCollection containing the photometry, its units, and methods for manipulating and visualising the photometry.
Once photometry has been generated it can be used to produce images; for more details see the [imaging docs](../imaging/imaging.rst).
In the pages below we demonstrate how to produce and use photometry.