Characterization of (CA)n microsatellite repeats from large-insert clones

The most laborious part of developing (CA)n microsatellite repeats as genetic markers is constructing DNA clones to permit determination of sequences flanking the microsatellites. When cosmids or large-insert phage clones are used as primary sources of (CA)n repeat markers, they have traditionally been subcloned into plasmid vectors such as pUC18 or M13 mp 18/19 cloning vectors to obtain fragments of suitable size for DNA sequencing. This unit presents an alternative approach whereby a set of degenerate sequencing primers that anneal directly to (CA)n microsatellites can be used to determine sequences that are inaccessible with vector-derived primers. Because the primers anneal to the repeat and not to the vector, they can be used with subclones containing inserts of several kilobases and should, in theory, always give sequence in the regions directly flanking the repeat. Degeneracy at the 3 end of each of these primers prevents elongation of primers that have annealed out-of-register. The most laborious part of developing (CA)n microsatellite repeats as genetic markers is constructing DNA clones to permit.