0004-077 = G158-027 [30]: H{alpha} emission is observed in the low-dispersion 
0004-077 FBS spectrwn.
0019-092 = G158-065 [30]. A trace of H{alpha} emission is seen.
0115-095 = G270-185 [32].
0134-070 = G271-110 [321.
0137-072 = G272-122 [32].
0200-110 = G272-143 [32].
0232-096 = GCCCS 378  [33].
0350-093 = SW Eri     [34].
0406-093 = GCCCS 611  [33] = Ste 85-21 [36].
0417-105 = AF Eri     [34].
0452-075 = NSV 01765  [37].
0452-070 = SX Eri     [34].
0453-097 = StM 86-38  [7].
0453-090 = NSV 01780  [37].
0828-108 = NSV 04114  [37].
0846-071 : a faint star (m_V_~14.5-15.0) of an early R subtype.
0853-089 : this object is not seen on Palomar E and O maps, while on the FBS 
0853-089 plate it is estimated to be a star of m_V_=13.0-14.0. Since the object 
0853-089 lies in the immediate vicinity of tbe star T Hya (i.e., the coordinates
0853-089 of the two objects are fairly close, {Delta}RA=0.3s & {Delta}DE=23.0"),
0853-089 automatic identification results in a false match with the source 
0853-089 PSC 08532-0857 [28], i.e., with T Hya [34]. The object is definitely 
0853-089 variable (an amplitude of at least 7.0").
0908-091 = VV Hya     [34].
0913-103 = G161-007 [32].
0939-086 = GCCCS 2591 [33].
1008-104 = StM86-136 [7].
1023-072 = StM86-138 [7].
1052-070 = G163-021 [32].
1053-091 = G163-023 [32].
1055-105 = LP731-76 [32]: a trace of H{alpha} emission is seen.
1059-073 = RT Crt [34].
1104-099 = GCCCS 2954 [33].
1118-108 = StM86-152 [7].
1130-103 = LRS87-89 [38]. The object is not seen on the Palomar O map. The 
1130-103 spectral range of about 6600-6900{AA} is seen on the FBS plate.  
1130-103 According to the low-dispersion classification [35] (LRS=44), the shell
1130-103 contains silicon carbide (SiC). There is probably a dense, gas-dust 
1130-103 shell around this object.
1148-069 = StM86-161 [7].
1238-086 = GCCCS3274 [33] = Ste85-70 [36]. Given as an object of m_V_=13.5 in 
1238-086 the catalog [36]. In accordance with the low-dispersion FBS spectrum, 
1238-086 this object can be classified as a star of middle R subtype.
1306-094 = TMSS-1027 [31]. According to Lewis et al. [39], this object is a 
1306-094 maser source.
1310-087 = TMSS-1028 [31]: a maser source according [39].
1339-070 : a star of m_V_=14.0-15.0. Judging from the energy distribution in the
1339-070 low-dispersion FBS spectrum, the subtype of this object can be assumed 
1339-070 to be between late R and early N.
1358-070 : this object is not seen on Palomar E and O maps. A very short part of
1358-070 the spectrum is seen on the FBS plate. Judging from the appearance of 
1358-070 the spectrum, the object can be assumed to be a star of late M subtype.
1358-070 It can be estimated to have m_V_=14.0-15.0 on the FBS plate.
1431-079 : an object of m_V_=13.5-14.5. A star of middle R subtype.
1434-080 : m_V_=14.5-15.5, a star of early R subtype.
1435-092 : a star of middle R subtype.
1438-087 = G124-061 [32].
1502-091 = StM86-214 [7].
1513-072 = G151-037  [32].
1536-068 = LDN 1778   [32].
1551-107 = TMSS-1032 [31].
1555-071 : in the APS digitized data base [40], this object is erroneously 
1555-071 classified as a galaxy. Probably a binary star.
1600-103 = V767 Sco   [34].
1610-085 = V558 Sco   [34].
1614-075 = V687 Oph   [34].
1615-080 = GCCCS 3680  [33].
1615-086 = V560 Sco   [34].
1618-090 = W Oph      [34].
1618-087 : an object of magnitude m_V_=13.0-14.0. In accordance with the 
1618-087 low-dispersion FBS spectrum, this object's subtype can tentatively be 
1618-087 assumed to be late R and early N.
2023-097 = SW Cap [34]. This object is given as a Mira Ceti variable in the 
2023-097 catalog of Kholopov et al. [34]. Only part of the spectrum (about 
2023-097 (about 6700-6900{AA}), which is very similar to that of a star of 
2023-097 subtype M8-M9, is seen on the FBS plate.
2032-076 = StM86-521 [7] = NSV 13155 [37].
2035-070 = V838 Aql [34].
2045-074 : a star of middle M subtype. On the FBS plate m_V_=13.0-14.0; this 
2045-074 object's type is erroneously given as a galaxy [40].
2055-109 = DG Aqr [34].
2058-076 = BZ Aqr [34] The APS [40] classification is erroneously given as a 
2058-076 galaxy. Probably a binary system.
2111-072 : estimated to be an object of m_V_=14.0-15.0 on the FBS plate. 
2111-072 The APS classification [40] is erroneous. Probably a binary system.
2120-073 = RZ Aqr [34].
2123-104 : estimated to be an object of m_V_~14.0-15.0 on the FBS plate. A star 
2123-104 of middle R subtype.
2207-095 : m_V_=13.0-14.0 on the FBS plate. A star of middle R subtype.
2249-110 = CE Aqr [34].
2252-072 = GCCCS 5761 [33].
2320-110 = SV Aqr [34].
2355-092 = V Cet [34].