In a thoroughgoing summary of new and historical observations of the symbiotic star YY Herculis, vsnet contributor Ulisse Munari and colleagues have provided a UBV sequence in the field (Munari et al. 1997, A&A 323, 113). The stars were observed using the Crimea 1.25-m telescope, but no details about the standard stars used is given. (Some of the U-B colors appear to be systematically too blue if the B-V's are correct.) Although a nice chart was provided for the field, no positions or identifications were given. These are shown in the table below. The first column shows the name assigned in the sequence by the authors. The positions were obtained from the GSC (v1.1), or for the two faintest stars, from the comprehensive USNO A1.0 star catalogue. I show a position for YY Her itself, since the coordinates in SIMBAD are only approximate (although not seriously in error). The two brightest sequence stars can be identified in the HDE. I also give V and B-V derived from Table 1 of Munari et al. Using the U-B and B-V colors, I show in lower case letters and in parens rough "predicted" spectral types for the fainter stars. The photoelectric sequence, by the way, shows that the values used on the charts by the AFOEV and by the AAVSO are okay for visual use except for the faintest stars. \Brian +++++++++++++++++++++++++++++++++++++++++ Munari et al.'s sequence near YY Herculis Name RA (2000) Dec GSC V B-V Remarks YY Her 18 14 34.2 +20 59 20 1579-0381 A 18 14 19.4 +21 02 50 1579-0482 11.21 0.49 HD 341876, F5 B 18 14 24.9 +21 05 21 1579-0136 11.60 0.47 HD 341875, G0 C 18 14 26.0 +21 01 12 1579-0432 12.06 0.60 (g0v) D 18 14 18.5 +20 56 46 1579-0364 12.40 0.93 (g8iii) E 18 14 33.9 +21 01 41 1579-0534 12.42 0.95 (g8iii) F 18 14 32.8 +20 55 39 1579-0518 12.18 1.03 (k0iii) G 18 14 26.5 +20 59 29 1579-0279 13.07 0.65 (g2v) H 18 14 46.7 +21 03 07 1579-0513 12.94 0.68 (g2v) I 18 14 45.0 +21 00 37 1579-0340 13.13 1.23 (k2iii) J 18 14 43.3 +21 00 48 1579-0525 13.61 0.94 (g8iii) K 18 14 24.5 +21 00 21 1579-0416 13.24 0.87 (k0v) L 18 14 30.5 +20 57 35 14.17 0.67 (g2v) M 18 14 38.8 +20 57 51 14.75 0.54 (f8v)