5: Spectrum B2III by Hiltner (1956ApJS....2..389H) 13: +59 611, published spectral type B0.5IV:nn. The nearby +59 612 13 is a previously known emission-line star. 13 The presumption would be that the emission in No. 13 is variable, 13 since the other, but not this one, was detected in the MWC survey. 18: BD magnitude 8.4. 22: Identified LS V 35 4: in Wackerling (1970MmRAS..73..153W), due to 22 the LS V labeling 35 4 rather than 35 5 as the BD star. 22 Other nomenclature is as in Wackerling (1970MmRAS..73..153W). 26: He I absorption lines visible in the blue at 280{AA}/mm. 28: H and K filled in? Hbet emission? 43: From the position, is variable BV 1618 Mon in IAU Var. Star Bull 921. 62: Listed as Half emission by Perraud, J. d. Obs., 44, 149, but 62 omitted by Wackerling (1970MmRAS..73..153W). 83: Missed in the SLS survey because it was slightly outside the 83 miscentered original SLS Half plate. 174: Henize evidently published this star with erroneous declination. 183: Just northward of Henize 144. 213: No. 529 in Table 15 of Wray's thesis Wray 1966; omitted by 213 Wackerling (1970MmRAS..73..153W). 228: In cluster NGC 37656. 233: Henize gives a position for a nearby brighter star, in which we 233 cannot see H{alpha} emission at lower spectral resolution than his. 246: Heidelberg 249, also No. 261 in a survey by Lynga, Arkiv f. Astr. 5, 246 No. 10 (OB stars). Half emission not previously reported. 254: No. 29 in a survey for OB stars by Lynga, Lund Medd., Ser. II, No. 141. 254 Half emission not reported previously. 265: Just northward of Henize 1110. 308: Not the nearby Henize 1411. 322: Not the nearby Henize 1482. 342: In cluster NGC 6520. 355: Strong ultraviolet continuum. 361: Near, but different from, Henize 1660. 368: The variable is listed as Mira-type. We see on our one red plate 368 no molecular-banded spectrum in the immediate, rather crowded, 368 vicinity. Near cluster OCl 44. 390: Comparison with the identification chart shows that this is 390 the nova-like star discussed by Dinerstein and Hoffleit in 390 IAU Var. Star Bull. No. 345; it is now named V3890 Sgr. 404: Half emission reported by The in Bosscha Contr. No. 14; 404 not in Wackerling (1970MmRAS..73..153W). 417: Not the nearby DQ Ser. 421: Half emission found by The, Bosscha Contr. No. 14, but omitted 421 by Wackerling (1970MmRAS..73..153W) because The classified the 421 spectrum as M1? Our red plate, somewhat more suitable for detecting 421 weak TiO than The's infrared plate, does not support this type. 428: Additional very weak emission lines in the red. AS 338, 428 not in Wackerling (1970MmRAS..73..153W). 430: A carbon star-No. 2703 in the general catalog (Publ. 430 Warner and Swasey Obs., 1, No. 4) is about 1' distant. 433: Our position is based on two accordant plates. Same star as 433 published by Krumenaker (1975PASP...87..185K), as shown 433 by his identification chart although he gives a position 433 about 0.1deg in error. Unknown to Krumenaker, the star had 433 been found and measured accurately (the Table 2 coordinates) 433 ten years earlier by Nassau and Stephenson. 438: Not the nearby AS 346. 441: Probably the star listed as at 19:30.0 by Bidelman and MacConnell 441 in 1973AJ.....78..687B, Table 3. 443: Our position does not agree very well with the published position 443 of the variable. We do not have the identification chart for it. 448: BD magnitude 9.3. 454: In cluster OCL 270.