The third set (charts 13 through 41) includes the complete collection of 4-meter plates, only slightly enlarged (1.05x) from the original plates. These make up the bulk of the atlas, covering virtually all of M31. Only a very few objects, including remote globular clusters, HI clouds, and satellite dwarf galaxies, lie beyond these charts.

Tables A-D in the appendix provide more detailed information on the individual objects identified on the charts. In the case of the globular clusters, we have used the Sargent et al. (1978) listing, which includes all previous discoveries. Table A gives the cluster number, its number in other catalogs, and the charts on which each cluster is identified.

Data on the open star clusters, based on the survey published by Hodge (1979), are presented in table B. In addition to the chart number, a coded description is given, using the following abbreviations:

L	=	large
s	=	small
f	=	faint stars only
m	=	moderately bright stars present
b	=	bright stars conspicuous
v	=	very

Table C lists the stellar associations in M31 that were identified by van den Bergh (1964). His numbers and association boundaries were taken directly from his published charts.

The dust clouds that were mapped and numbered by Hodge (1980) are listed in table D. As is mentioned in that reference, the separation of dust regions into discrete clouds is somewhat arbitrary and done for the convenience that such identifications provide. Many separately-numbered objects are clearly seen to be connected and interlaced on appropriately-exposed plates; any physical interpretation of the plotted dust cloud boundaries must be very tentative. A proper detailed multicolor study would be necessary in order to disentangle the physical structure of any particular dust region.