... one

Based in part on observations obtained at the European Southern Observatory using the ESO Very Large Telescope on Cerro Paranal (ESO program 166.A-0701). Based in part on observations obtained at the Hale Telescope, Palomar Observatory, as part of a continuing collaboration between the California Institute of Technology, NASA/JPL, and Cornell University.

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...(Balogh et al. 2001)

The MF from Balogh et al. (2001) was calculated with a Kennicutt IMF, so we applied a correction $\log M_{\rm stars}^{\rm salpeter} = \log M_{\rm stars}^{\rm kennicutt} +0.35$.

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