LFs by spectral type
For 12,000 galaxies with PCA types, fit LFs by type.
1/Vmax LFs have less-steep faint ends than STY fits of Schechter functions.
From early to late types…
- M* gets fainter: -19.6 ? -18.9
- ? gets steeper: -0.7 ? -1.7
Overall M* brighter than M* of any type; Schechter function not adequate fit.
Evidence for upturn at faint end of LF.