This appendix contains data on extragalactic globular clusters systems and their host galaxies. These data are used extensively in Chapters 5 and 6 for studying trends and correlations in these properties. Similar information can be found in Harris and Harris (1997) and Kissler-Patig (1997).

An asterisk after the galaxy number indicates that less than 10% of the estimated number of globular clusters in that galaxy have been observed. All galaxy numbers are NGC numbers unless otherwise specified.

The sources listed in the right-hand column can be found in the references of the main text through the following key:

Ba95, Baum et al (1995); B195, Blakeslee and Tonry (1995); Bo92, Bothun et al. (1992); Br92, Bridges and Hanes (1992); Br94, Bridges and Hanes (1994); Br96, Bridges et al. (1996); Br97, Bridges et al .(1997) Bu92, Butterworth and Harris (1992); Ch3, chapter 3 of this book; Ch4, chapter 4 of this book Ch93, Christian (1993) Di96, Dirsch (1996); Du96a, Durrell et al .(1996a), Du96b, Durrell et al .(1996b); F195, Fleming et al .(1995), Fo96; Forbes et al .(1996); Ge96, Geisler et al .(1996); H91, Harris (1991); Ha92, Harris et al .(1992); Ha95, Harris et al .(1995); Ho95, Hopp et al .(1995); Hi96, Hilker and Kissler-Patig (1996); Ka96, Kaisler et al .(1996); Ki94, Kissler et al .(1994); KP96, Kissler-Patig et al .(1996); KP97, Kissler-Patig et al .(1997); Le94, Lee et al .(1994) McL94, McLaughlin et al .(1994); McL95, McLaughlin et al .(1995); Os93, Ostrov et al (1993); Pe95, Perelmutter and Racine (1995); Ri92, Richtler et al (1992); Se95, Seeker et al (1995); Sh93, Schommer (1993); Sc93, Suntzeff (1993); W97, Whitmore et al (1997) Ze94, Zepf et al (1994), Ze95, Zepf et al (1995).