Here are electronic versions of different data sets used in various papers. Please drop me an e-mail if you have any questions or problems.

• Bell et al. 2012: Rest-frame quantities and stellar masses for galaxies from the Williams et al. 2009 UDS dataset
• Borch et al. 2006: Mass function data points for all galaxies, blue cloud galaxies, and red sequence galaxies
• Bell et al. 2004: Luminosity function data points for the 5000 red-sequence galaxies paper.
• Bell & de Jong 2000: Radially resolved color profiles for sample galaxies in the large bins for colour-colour plots, along with physical parameters.
• Bell et al. 2003: Global parameters (structural parameters and B-R and R-K colors at the half-light radius) for Bell & de Jong 2000 sample galaxies.
• Bell 2002: Data (FUV extinction, beta, Ha/FUV and FUV-B color) for the short paper on the difficulties of using beta as an extinction indicator for normal star-forming galaxies.

My SDSS work with McIntosh, Katz and M. Weinberg:

• Stellar, HI and H2 masses for EDR galaxies
• k and evolution corrections for EDR galaxies
• k corrections only for EDR galaxies
• u-band LF
• g-band LF
  • late types by concentration
  • early types by concentration
  • late types by color
  • early types by color
• r-band LF
• i-band LF
• z-band LF
• K-band LF
  • late types by concentration
  • early types by concentration
• Predicted K-band LF – see the text of the paper for the hybrid Schecter+power-law fit
• K-band stellar mass function – ‘diet’ Salpeter IMF
  • late types by concentration
  • early types by concentration
  • g-band LF
• • late types by concentration
  • early types by concentration
  • late types by color
  • early types by color
• g-band distribution of stellar M/L
• K-band distribution of stellar M/L
• Baryonic mass function assuming diet Salpeter
• Baryonic mass function assuming Kennicutt/Kroupa
• Baryonic mass function assuming ‘Bottema IMF’
• Predicted atomic hydrogen mass function
• Predicted molecular hydrogen mass function