Bob Modic, attentive as usual, has noticed that I have identified in error the mag. 12.6 star observed by Tsvetkov near NGC 2841. Using his information, I have made the correct ID, confirmed by offsets for another star in Tsvetkov's list that is farther afield. The complete revised sequence list is given again below. Below the main table is a list of explicit R magnitudes for each star that might be suitable for ordinary unfiltered CCD systems. The last line shows magnitudes for the "new" Tsvetkov star in the GSC and USNO-A2.0 catalogues. I got a note today from Harold Corwin, who observed the BVRI sequence with Marian Frueh. (If I previously gave the impression that the stars were observed by me, that was not my intention---the material is merely unpublished.) Harold noted that he thought the stars in this field were adequately measured except perhaps the faintest stars in the U (not given here) and I filters. \Brian Name RA (2000) Dec s GSC V B-V V-R V-I NGC 2841 1 9 22 28.4 +51 00 51 G 3431-0219 8.48 1.29 0.67 1.23 NGC 2841 2 9 21 50.8 +51 00 36 G 3431-0625 11.07 0.59 0.33 0.65 NGC 2841 3Ts 9 22 53.3 +51 01 28 G 3431-1249 12.62 0.64 (0.37) NGC 2841 3 9 21 47.3 +50 58 50 G 3431-0053 13.51 0.75 0.43 0.83 NGC 2841 4 9 21 58.2 +51 00 16 G 3431-0495 13.77 0.60 0.40 0.74 NGC 2841 5 9 22 02.3 +51 01 23 G 3431-0159 14.19 0.83 0.42 0.91 NGC 2841 147 9 22 06.8 +50 53 37 G 3431-0802 14.72 0.88 (0.49) Note: V-R colors in parens were derived from B-V. Name R 1 7.81 2 10.74 3Ts 12.25 3 13.08 4 13.37 5 13.77 147 14.23 In photographic catalogues, 3Ts: m(GSC)=12.58, USNO-A2.0 mb=13.3, mr=12.3