0029+0509  The identification given by Lawrence et al. (1986ApJS...61..105L); 
0029+0509  stellar source B=20.0, R=19.0, shifted by 0.6arcsec from the 
0029+0509  radio position.
0034+0514  The shape of the object suggests "precession".
0039+0454  Lawrence et al., 1986ApJS...61..105L also give on POSS an empty 
0039+0454   field at the radio source position.
0042+0504  Probably a quasar.
0043+0502  The same as in the case of 0039+0454.
0103+0524  Chigo (1977ApJS...35..359G) identified the source with a V=19.5 
0103+0524   magnitude optical object.
0126+0502  Probably a quasar.
0143+0505  The first optical candidate is probably a quasar, the second one is 
0143+0505   the galaxy near the N-component of the radio image.
0226+0512  Probably a quasar.
0234+0446  The source was identified by Bugaenko et al. (1993PAZh...19...13B), 
0234+0446   U=18.4, U-B=-0.7, B-V=0.3, V-R<-0.6. According to Veron-Cetty, 
0234+0446   Veron (1993, Cat. <VII/166>) this quasar with V=18.5 is at the 
0234+0446   redshift z=2.06.
0318+0506  In Lawrence et al. (1986ApJS...61..105L) the source seems double, the
0318+0506   NE component is lost on the VLA snapshot map.
0324+0442  This source is identical to the USS source 0321+045 observed with a 
0324+0442   better resolution by Rottgering et al. (1994A&AS..108...79R). Our 
0324+0442   bright component is split on three ones marked in the CCD image 
0324+0442   (Fig.9). The middle component is the brightest one. It coincides 
0324+0442   with our bright component within 0.5arcsec.
0343+0458  The centroid of the double source of UTRAO catalog is between the two
0343+0458   listed components, although the position of the second component is 
0343+0458   under a question. The redshift of the source is z=0.358 (Spinrad et 
0343+0458   al., 1985PASP...97..932S). Veron-Cetty, Veron (1993, Cat. <VII/166>)
0343+0458   gives for this galaxy V=19.17, B-V=0.35, U-B=-0.5.
0446+0525  The weak core is possible. Accoriding to Lawrence et al. 
0446+0525   (1986ApJS...61..105L) the field is also empty.
0505+0459  According to Bugaenko et al. (1993PAZh...19...13B) the colors of the 
0505+0459   source are U=19.0, U-B=0.0, B-V>02.
0519+0510  Complicated structure, indicating either precession of object or 
0519+0510   repeated activity which leads to the second ejection from a core.
0619+0506  Bad cleaning of the VLA map. It's difficult to determine the source 
0619+0506   structure.
0621+0437  Bad cleaning of the map. The centroid of the asymmetric double source
0621+0437   of the UTRAO catalog (R.A.=6h19m13.71s, Dec=4{deg}40'04.33") is 
0621+0437   shiftted to NE. Weak extended structures are lost on the VLA maps 
0621+0437   with a high resolution, so the real radio structure of the object 
0621+0437   most likely differs from that in the mentioned map and in Lawrence 
0621+0437   et al. (1986ApJS...61..105L). An empty field on POSS of Lawrence et 
0621+0437   al. (1986ApJS...61..105L) agrees with our statement. The VLA data 
0621+0437   with the 45arcsec resolution at 1400MHz (NRAO/VLA Sky Survey (NVSS) 
0621+0437   radio source catalog) show two radio components (see Table 2). The 
0621+0437   centroid of this source coincides with the UTRAO coordinates. The 
0621+0437   object is identified with the optical galaxy with m_R_ equal 
0621+0437   approximately to 18.5.
0653+0508  This source is a point one in Lawrence et al. (1986ApJS...61..105L) 
0653+0508   and in UTRAO catalog. Identification in Lawrence et al. 
0653+0508   (1986ApJS...61..105L) agrees with the mentioned one in Table 2.
0759+0454  Empty field is not excluded.
0809+0500  The source is identified with the one of three unresolved galaxies. 
0809+0500   On the POSS some filaments emerged from this galaxy are seen.
0907+0439  Identification in Lawrence et al. (1986ApJS...61..105L) agrees with 
0907+0439   the mentioned one in Table 3.
0937+0450  The centroid of the double UTRAO catalog source has 
0937+0450   R.A.=9h34m33.356s, Dec=5{deg}03'38.58", so the extended component 
0937+0450   and possibly the second one are lost on the VLA map. Only one 
0937+0450   component is on the mentioned map.
0949+0454  The position and the radio image of the source have been taken from 
0949+0454   Lawrence et al. (1986ApJS...61..105L). The identification agrees 
0949+0454   with ours.
1016+0514  The source in Lawrence et al. (1986ApJS...61..105L) is a point one 
1016+0514   and identified with the stellar object with B=20.0, R=20.5 shifted 
1016+0514   by 0.3arcsec from the radio source.
1045+0455  Empty field on POSS is in agreement with Lawrence et al. 
1045+0455   (1986ApJS...61..105L).
1049+0506  The source was identified with the quasar with V=18.94, B-V=0.24, 
1049+0506   U-B=-0.88 at the redshift z=1.115 (Veron-Cetty, Veron, 1993, 
1049+0506   Cat. <VII/166>).
1102+0459  The double source in the UTRAO catalog (with centroid 
1102+0459   R.A.=11h00m11.117s and Dec=5{deg}03'38.58") is situated near the 
1102+0459   weak point component (R.A.=11h00m11.02s and Dec=5{deg}15'21.19") 
1102+0459   which most likely is a core of this object. There is only the NE 
1102+0459   component on the VLA map.
1124+0456  Bad cleaning of the VLA map. Weak extensive details are possibly 
1124+0456   lost.
1131+0455  The well known gravitational lens.
1145+0455  Bugaenko et al. (1993PAZh...19...13B) identified this source with the
1145+0455   object with U=18.5, U-B=0.2, B-V=0.0, V-R<0.5. Veron-Cetty, Veron 
1145+0455   (1993, Cat. <VII/166>) give for this quasar V=19.5, the redshift 
1145+0455   z=1.342.
1148+0459  The central component is a core with a jet. This source is a cometary
1148+0459   one in Lawrence et al.  (1986ApJS...61..105L). Identification (empty
1148+0459   field on POSS) agrees with ours.
1154+0431  Probably a quasar.
1218+0515  Complicated structure source. The source is elongated in one 
1218+0515   direction; probably a core exists.
1226+0438  The centroid of the asymmetrical double source from the UTRAO catalog
1226+0438   has R.A.=12h24m21.94s, Dec=4{deg}45'40.84", so only SE component of 
1226+0438   the object is possibly seen on the VLA map. That's why the 
1226+0438   identification in Lawrence et al. (1986ApJS...61..105L) with the 
1226+0438   stellar object with B=21.0, R=20.5, shifted by 0.4arcsec, is 
1226+0438   probably unreal.
1239+0443  The identification in Lawrence et al. (1986ApJS...61..105L) (empty 
1239+0443   field on POSS) differs form ours (see Table 3)
1257+0458  Bad cleaning of the VLA map. The real image of the object is unknown.
1340+0448  The point source coincides with the IRAS source in the box of errors 
1340+0448   and with the optical galaxy REIZ 3561 (MCG +01-35-028; ZWG 045.068).
1347+0435  Bad cleaning of the VLA map; complicated morphology.
1356+0457  Complicated structure; there are two bright components. The object is
1356+0457   identified with the galaxy NGC 5364 (Hummel, 1980A&AS...41..151H; 
1356+0457   Dressel, Condon, 1978ApJS...36...53D; Condon, 1987ApJS...65..485C).
1424+0442  Identified by Bugaenko et al. (1993PAZh...19...13B) with the object 
1424+0442   with U=18.0, U-B=-0.3, B-V=0.2, V-R=1.0.
1436+0501  Complicated structure; precession of the object is possible.
1446+0507  Bad cleaning of the VLA map. Extended structure of the object is 
1446+0507   possibly lost. The identification of Lawrence et al. 
1446+0507   (1986ApJS...61..105L) (empty field) differs from ours.
1526+0514  Bad cleaning of the VLA map. The centroid of the double UTRAO catalog
1526+0514   source has R.A.=15h23m30.515s, Dec=5{deg}20'41.1". This source has a
1526+0514   cometary structure in Lawrence et al. (1986ApJS...61..105L) and the 
1526+0514   identification is also an empty field.
1543+0452  Bugaenko et al. (1993PAZh...19...13B) give for the identified object 
1543+0452   U=15.1. It is Zwicky galaxy.
1550+0524  Veron-Cetty, Veron (1991ESOSR..11....1V) give for this source z=1.422
1550+0524   and V=17.7.
1559+0502  Bad cleaning of the VLA map. There is a bright core with weak 
1559+0502   components around it.
1616+0459  Veron-Cetty, Veron (1991ESOSR..11....1V) give for this quasar V=19.5 
1616+0459   and redshift z=3.209.
1658+0514  Although the source is double, the second component is very weak, so 
1658+0514   this object is either a core with a jet or these are two independent
1658+0514   sources. Veron-Cetty, Veron (1991ESOSR..11....1V) give for this 
1658+0514   quasar redshift z=0.879, V=16.54, B-V=0.46, U-B=-0.6. This quasar is
1658+0514   also an X-ray source.
1728+0429  The source is identified with a quasar with V=16.99, B-V=0.44, 
1728+0429   U-B=-0.56 at the redshift z=0.293. This source is also an X-ray 
1728+0429   source (Veron-Cetty, Veron, 1993, Cat. <VII/166>).
1754+0459  The position and the radio image of the object have been taken from 
1754+0459   Lawrence et al. (1986ApJS...61..105L); they give an empty field or 
1754+0459   possible identification with the object with m=17.5. Our measurement
1754+0459   demonstrates the reality of the last identification.
1806+0527  The coordinates and the radio map of the source have been taken from 
1806+0527   Lawrence et al. (1986ApJS...61..105L). The source may be a core with
1806+0527   two jets or a double source of FRII type.
1829+0451  Side by side is the object with R=20.0 with the coordinates: 
1829+0451   R.A.=18h27m30.78s, Dec=4{deg}50'25.3".
2029+0456  Lawrence et al. (1986ApJS...61..105L) identified this source with the
2029+0456   fuzzy object, shifted by 1.4arcsec, with B=21.0, R=20.5.
2044+0444  Bad cleaning of the VLA map.
2110+0505b Borisov (1991, priv. comm.) identified this source with the quasar 
2110+0505b  with z=2.95.
2116+0507  This source is identified with a quasar with V=20.37 at the redshift 
2116+0507   z=1.001. The source radiates in the X-ray band (Veron-Cetty, 
2116+0507   Veron, 1993, Cat. <VII/166>).
2117+0503  Identification of Lawrence et al. (1986ApJS...61..105L) (empty field)
2117+0503   agrees with ours.
2204+0442  Bugaenko et al. (1993PAZh...19...13B) identified this source with the
2204+0442   object with U=12.6, U-B=0.4, B-V=1.9, V-R=0.8. Veron-Cetty, Veron 
2204+0442   (1993, Cat. <VII/166>) give for this galaxy V=15.2, B-V=1.0, 
2204+0442   U-B=0.22 and the redshift z=0.098.
2144+0513  The first optical candidate is probably a quasar, the second one is a
2144+0513   galaxy.
2224+0513  An extended component is possibly lost. Lawrence et al. 
2224+0513   (1986ApJS...61..105L) give for this source an empty field.
2225+0523  This source has a cometary structure in Lawrence et al. 
2225+0523   (1986ApJS...61..105L); the identification with the stellar object 
2225+0523   shifted by 0.3arcsec with B=18.0, R=18.5. Veron-Cetty and Veron 
2225+0523   (1991ESOSR..11....1V) give the redshift z=2.323. 
2245+0501  Bugaenko et al. (1993PAZh...19...13B) give for the identified object 
2245+0501   U=19.3, U-B=0.0, B-V=0.3, V-R=1.5.
2258+0517  Lawrence et al. (1986ApJS...61..105L) give for this source an empty 
2258+0517   field.
2320+0512  The source is identified with the quasar with V=19 at the redshift 
2320+0512   z=0.623 (Veron-Cetty, Veron, 1993, Cat. <VII/166>).
2343+0520  Lawrence et al. (1986ApJS...61..105L) identified this source with the
2343+0520   stellar object shifted by 0.9arcsec with B=19.5, R=20.0.