00:52:25.9   Sto V-4, no. 16 in the 1st ed. of the S-star catalog.  Weak carbon according to Feast  
             et al, Obs. 97, 140, 1977.                                                             
01:20.4      D 209.  No Case plates.  A visual double in the Case 36" Cassegrain, 9" in 315d.   
             Mag. difference approx. .5 mag.                                                        
02:46.1      S 52.  A different star from the nearby S 51.  Any ZrO that may be present is too weak 
             to make this star interesting.                                                         
03:03:41.6   Sto V-44.  This appears to be LTT 1479, an M dwarf.  It is also a Luyten double star,  
             but the cpm companion is more distant than the nearby star mentioned by Sto.           
04:14.1      SX Cam. K's classification was a quote from Bidelman, who later decided (Bid65) that he
             had taken the wrong star, viz. no. 90 of this catalog.  On an infrared objective prism 
             plate I confirm the Bid65 spectral type of late M for SX Cam.                          
06:39.5      Same as another star in the same discovery paper; declination sign should be minus.    
             Corrected in Abast. Bull. 47, 10.                                                      
07:49:36.4   No. 942 in my carbon star catalog, 1st ed.                                             
08:36:07.3   No. 1253 in my carbon star catalog, 1st ed.                                            
08:46:16.3   Sto IV-12. No. 1309 in the 1st ed. of my carbon star catalog; subsequently confirmed as
             such on a 10-degree red objective prism plate (MacCon, Ste).                           
09:50:00.3   Wray 173.  No. 18 in the catalog of Wolf-Rayet stars by Roberts, Astron. J. 67, 79,    
             1962.  L. Smith, Monthly Not. Roy. Astron. Soc. 138, 109, 1968 finds B9e? from a slit  
             spectrogram.  Henize, Astrophys. J. Suppl. 30, 491, 1976 suggests that a planetary neb-
             ula is involved.  On a Tololo red-region plate I find a possible weak H alpha emission 
             overlapping an early-type spectrum.                                                    
13:38:50.1   Sto IV-50.  This seems to be LTT 5330, a probable M dwarf.                             
16:45.3      Henun 169.  Reclassified in Rybski's thesis; should have been included in my rejected S
             stars table in the 1st ed. of this catalog.                                            
17:07:49     TV Dra.  The Balz reference is to McCormick Publ. Vol. 13, part 1.                     
17:19:48     ST Ser.  I do not know the source of the GCVS spectral type.                           
17:53:56     HR 6702 = OP Her = HD 163990(Mb).  Reclassified M5 IIb-IIIa by Keenan in Basic Astrono-
             mical Data.                                                                            
18:02:02     VX Sgr.  My red plates, several in number, are all overexposed.                        
18:05.7      S-WS 5.  No. 2544 in the 1st ed. of my carbon star catalog.                            
18:08:16.2   No. 549 in the 1st ed. of the S-star catalog, and no. 2552 in the 1st carbon star cata-
             log.  Originally classified S from a red objective prism plate, on which it was however
             peculiar; looks much the same way on a recent one, and not very S-like.  Looks like a  
             carbon star on the 3400 A/mm infrared objective prism plate used for that original dis-
             covery, but not on four others including one recent one.  No secure evidence for light 
             variability.                                                                           
18:24.0      D 4847.  Appears to be either T Ser or BN Ser, both of which are M stars (5).          
20:00:44.0   Included as S by NassSte through clerical error; it is an H alpha-emission star, and   
             slipped into the wrong list.                                                           
20:35.6      S-WS 64.  Reddened M according to Pesch, Astrophys. J. 149, L65, 1967; M4 by Vogt,     
             Astron. J. 78, 389, 1973.                                                              
21:00.7      RV Aqr.  A good N star, no. 2968 in my carbon star catalog 1st ed.  The Dearborn obser-
             vers thought the red-region spectrum resembled that of GP Ori (SC).                    
22:44.6      S-WS 43.  The S-WS position was derived by offsetting from a nearby B.D. star, but the 
             B.D. number quoted for it is nowhere near the published S-star position.  I have also  
             examined spectral plates covering the position exactly 1h of r.a. different from this, 
             with equal lack of success.