As far as I know, there is no published photometric sequence around M96. On the relevant chart from the Thompson & Bryan "Supernova Search Charts" are shown V magnitudes evidently from several professional observers. Below are the positions and IDs for these stars (except a faint star very close to the galaxy). The name indicates the magnitude rounded to 0.1, e.g. "114" means V = 11.4. ID RA (2000) Dec GSC 114 10 46 23.9 +11 56 54 0849-0685 126 10 46 21.7 +11 44 29 0849-0703 131 10 46 32.7 +11 50 55 0849-0841 135 10 46 10.4 +11 42 50 0849-0887 143 10 46 52.9 +11 43 22 0849-0306 149 10 46 52.9 +11 52 42 0849-0206 150 10 46 32.7 +11 52 06 0849-0931 T&B give the sources for this data as Peter Birch et al. (Perth Observatory, Western Australia), Bill Liller and Gonzalo Alcaino (CTIO?), and Marion Frueh (probably McDonald Observatory). Since I complain that the IAUC's don't give a precise position for the host galaxies of supernovae, the center of M96 is at: 10 46 45.6 +11 49 18 (2000), according to NED, which cites 1996 ApJS 107, 215, and claims an accuracy of +/- 5 arcsec. \Brian