“…First, we tested 38 microsatellite loci that have been successfully amplified in other hoofed species: Bos taurus-BM1258 (Hediger et al 1991), BovirBP, MM12 (Moore et al 1992), MAF46 (Swarbrick et al 1992), INRA003 (Vaiman et al 1992), INRA35 (Steffen et al 1993), TGLA53 , BL42, BM1225, BM2830, BM4513, BM861, BM888, BMC1009, IOBT965 (Bishop et al 1994), CSSM003 , INRA124 (Vaiman et al 1994), Haut14 (Thieven et al 1995), INRA189 (Kappes et al 1997), UMN2404 (Liu et al 2002), and UMN2001 (Liu et al 2003); Cervus elaphus-CelJP15 (Pemberton et al 1995); Odocoileus virginianus-Cer14 (DeWoody et al 1995); Ovis aries-MAF70 (Buchanan and Crawford 1992), OarFCB193, OarFCB304 (Buchanan and Crawford 1993), OarFCB20 (Buchanan et al 1994), McM58, andMcM130 (Hulme et al 1994); and Rangifer tarandus-RT5, RT9, RT23, RT24, RT27, RT30 (Wilson et al 1997), NVHR T01, NVHRT21, and NVHRT24 (Røed and Midthjell 1998) (Table 5S1 and Table 6S2). Markers were selected on the basis of their previous cross-species utility, size range, and ability to co-amplify in multiplex PCRs.…”