1 Near a known emision line galaxy, separately seen on the survey plate 2 Spectrum M3; an NLTT star, hence dMe, but the dwarf character is not 2 apparent on my plate 25 In the Taurus dark cloud 26 In the Taurus dark cloud 28 In the Taurus dark cloud; 11" double (Romano, 1975 Ap. Space Sci., 33, 487) 31 In the Hyades field 36 H{alpha} emission somewhat diffuse 37 Doubtless V534 Ori 44 Also HeI {lambda}6678? 49 Not the nearby V380 Ori, which is also visible on the same plate. The 49 Dixon-Sonneborn (1980, A Master list of Nonstellar Optical Astronomical 49 Objects, Columbus: Ohio State University Press) catalog lists many 49 Herbig-Haro objects near this position 52 CSV 6386 67 Another emission line, stronger than the H{alpha}, is present, 67 perhaps HeI {lambda}6678 79 No continuum on the survey plate. The Palomar red survey print shows a very 79 faint star, far below my plate limit, in or very near this position. 82 CW UMa, also seen on my plate is 1.5' away 83 The H{alpha} emission is somewhat diffuse, on a stellar continuum 88 This appears to be an otherwise featureless continuum near the plate limit, 88 with H{alpha} emission several tens of Angstroems broad. A direct plate 88 shows that it is not a spectrum overlap. 100 Either the emission does not belong to the accompanying continuum, or it 100 is redshifted. 101 A second emission, probably HeI {lambda}6678, is present 124 The emission may not belong to the star whose continuum is visible 126 In Ophiuchus dark cloud 127 In Ophiuchus dark cloud 128 In Ophiuchus dark cloud 129 In Ophiuchus dark cloud 130 In Ophiuchus dark cloud 132 Perhaps also HeI {lambda}6678. 153 Perhaps also HeI {lambda}6678. 156 Not the nearby V2068 Sgr, which appears also on my plate 157 Evidently BPM 93781, even though the declinations differ by 7'; the Lick 157 Sky Atlas (Shane & Wirtanan, 1959) shows no other candidate for the 157 BPM star. 178 LS III+54.4 189 Independently discovered as Be by Bidelman (1985AJ.....90..341B) 190 Probably symbiotic. Shows H{alpha}, H{beta} He D3, and N_1_, N_2_ on a very 190 red continuum. 193 NSV 13903 has a published position quite nearby but is supposed to be an 193 M star (as well as possible Mira variable). The present star is 193 emphatically neither M-type nor even red. I do not find a candidate for the 193 NSV star. 194 BD+53 2748, an M star, is nearby. Should have been included in Stepheson 194 and Sanduleak's list (1977, Cat. ) 1r near to but not same as emission-line galaxy NGC 59; 1r ID uncer due to Stephenson +16" Dec error(?). 16r Southwestern star of 16" pair; Downes & Keyes (1988AJ.....96..777D) 16r identify this incorrectly as the northeastern star. 28r Southeastern star of 11" pair; Downes & Keyes (1988AJ.....96..777D) 28r identify this incorrectly as the fainter northwestern star. 44r Also emission at HeI 6678A? 45r NSV 16355 = [AD95] 2455. 46r Southwestern star of 18" pair. 67r Another em. line stronger than H-alpha, possibly HeI 6678A. 79r No continuum, vf on POSS red print. spectral type F7 is for 79r Nearby star (2003A&A...402..963M), not Stephenson object. 79r very red Sloan colors and modest USNO-B1.0 proper motion suggest 79r this could be an M-dwarf flare star. 83r Emission somewhat diffuse on stellar continuum. 88r Ste -27" Dec error; H-alf several tens of Angstroms wide on 88r featureless continuum near plate limit. 100r Either emission does not belong to accompanying cont. or it is redshifted. 128r Also CRBR 2315.5-1337. 147r -1 deg Dec error in on-line file. 149r also ROTSE1 J181855.69+272627.9. 153r WR-like, perhaps also HeI 6678A em. 157r BPM 93781 with -7' Dec error? 190r Symbiotic w/H-alf,bet,He D3, [OIII] doublet on vred continuum.