WillHartley

## Description The k-correct stellar mass (formed) provides a convenient way to quantify the SED amplitude, as it depends directly on the mass. However, making this assumption in SkyPy prevents...

### Discussed in https://github.com/skypyproject/skypy/discussions/536 Originally posted by **WillHartley** March 24, 2022 In the k-correct templates we have the mass in stars formed, and the mass remaining (after mass loss due...

Forced-photometry mode(s)

5

We've discussed this a few times, and I've promised to write up the issue for some time. Here it (finally) is. A common approach to measuring multi-band photometry is to...