Candidate RR Lyrae stars found in Sloan Digital Sky Survey commissioning data

We present a sample of 148 candidate RR Lyrae stars selected from Sloan Dig ital Sky Survey (SDSS) commissioning data for about 100 deg(2) of sky surve yed twice with Delta t = 1.9946 days. Although the faint-magnitude limit of the SDSS allows us to detect RR Lyrae stars to large Galactocentric distan ces (similar to 100 kpc, or r* similar to 21), we find no candidates fainte r than r* similar to 20, i.e., farther than similar to 65 kpc from the Gala ctic center. On the assumption that all 148 candidates are indeed RR Lyrae stars (contamination by other species of variable star is probably less tha n 10%), we find that their volume density has roughly a power-law dependenc e on Galactocentric radius, R-2.7+/-0.2, between 10 and 50 kpc and drops ab ruptly at R similar to 50-60 kPc, possibly indicating a sharp edge to the s tellar halo as traced by RR Lyrae stars. The Galactic distribution of stars in this sample is very inhomogeneous and shows a clump of over 70 stars at about 45 kpc from the Galactic center. This clump is also detected in the distribution of nonvariable objects with RR Lyrae star colors. When sources in the clump are excluded, the best power-law fit becomes consistent with the R-3 distribution found from surveys of bright RR Lyrae stars. These res ults imply that the halo contains clumpy overdensities inhomogeneously dist ributed within a smooth R-3 background, with a possible cutoff at similar t o 50 kpc.