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{\bf Notes to individual sources in Table 3}
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{\bf 0717+367:} in Abell cluster 579

{\bf 0722+393:} Confusing, flat-spectrum, possibly variable source at 
$07^{h}26^{m}04.^{s}8; +32^{o}12'28"$ (5.8 arc min away). $S_{1.4}\approx 135-210$ mJy

{\bf 0723+488:} A featureless optical spectrum  was observed in March 1992 with the 
Asiago 182-cm telescope (cf. Machalski 1992). Variable in the radio (cf. Table 3) 
and likely in the optical

{\bf 0751+485:} A featureless optical spectrum was observed in March 1992 with 
the Asiago 182-cm telescope (cf. Machalski 1992)

{\bf 0755+379:} NGC2484; UGC4125. References to WSRT maps and physical parameters 
in Condon \& Broderick (1988)

{\bf 0755+480A:} Confusing, extended, double source 0755+480B (3.0 arc min away), 
identified with a faint galaxy

{\bf 0804+499A:} 8.4 arc min apart from very compact variable quasar 0804+499B

{\bf 0804+370:} Confusing source at$08^{h}08^{m}29.^{s}44; +36^{o}59'43"7$, 
$S_{1.4}\approx 60$ mJy 

{\bf 0809+328:} The radio source is likely associated with one of two close 
(separation of 2.3 arc sec) galaxies in a pair

{\bf 0810+351:} Centroid of the double radio source coincides well with the 
bright elliptical galaxy, however morphological type of the source with evident 
bright 'hot spots' is not typical for galaxies at $z<0.1$

{\bf 0816+367:} Confusing  flat-spectrum source at $08^{h}20^{m}20.^{s}2;$ 
$+36^{o}40'05"$ (4.5 arc min away). $S_{1.4}\approx 100$ mJy

{\bf 0818+472:} Two confusing sources: $S_{1.4}\approx 190$ mJy at 
$08^{h}21^{m}59.^{s}0; +47^{o}02'53"$ (5.2 arc min away), and $S_{1.4}=54$ mJy, 
flat-spectrum, at $08^{h}22^{m}09.^{s}6; +47^{o}05'53"$ (6.9 arc min away)

{\bf 0822+394:} The spectrum breaks at about 1.4 GHz. Low-- and high--frequency 
spectral indices differ significantly: $\alpha _{0.4}^{1.4}\approx 0.42$, 
$\alpha_{1.4}^{10}\approx 1.14$

{\bf 0829+512:} Neither of two suggested galaxy identifications (cf. Paper III) 
is convincing, however association of the radio source with a faint distant 
galaxy is very probable

{\bf 0838+325:} in Abell cluster 694/695.  4885-MHz VLA map of the central part 
of the source is shown in Figure A1 (Appendix)

{\bf 0844+319:} IC2402 galaxy

{\bf 0906+480A:} Close pair (4.3 arc min apart) with 0906+480B. Both are very 
compact; deconvolved size of $0.0 \times 0.0$ arc sec at 5 GHz. Spectral indices 
quoted in Paper IV and Machalski \& Inoue (1990) were erroneously interchanged. 
Probably variable above 5 GHz

{\bf 0908+380:} Confusing, steep-spectrum source (0908+380B in the B3VLA sample; 
Vigotti et al. 1989) at $09^{h}11^{m}48.^{s}5; +37^{o}50'19"$ (3.1 arc min away). 
$S_{1.4}\approx 150$ mJy

{\bf 0910+353:} The VLA A-array map and optical identification of the source 
published in Paper IV were wrong. The correct map reproduced from the FIRST survey 
(courtesy of R.H. Becker) with the new identification indicated is shown in 
Figure A2 (Appendix)

{\bf 0911+354:} Northern component with $S_{1.4}\approx 50$ mJy (cf. VLA A-array 
map in Paper IV) may be a separate source

{\bf 0918+381:} Confusing, very steep-spectrum, double source 0919+381 at 
$09^{h}22^{m}15.^{s}20; +37^{o}54'03"$ (6.9 arc min away). $S_{1.4}=295\pm 6$ mJy

{\bf 0927+352:} Radio, optical, and X-ray properties of the source are discussed 
in Machalski \& Brandt (1996)

{\bf 0928+480:} Southern component at $09^{h}31^{m}34.^{s}3; +47^{o}49'47"$ 
(marked 'B' in Paper II) is likely a separate source. $S_{1.4}=186$ mJy in NVSS

{\bf 0949+354:} Confusing, flat-spectrum source at $09^{h}52^{m}22.^{s}6; 
+35^{o}08'03"$ (5.2 arc min away). $S_{1.4}\approx 50$ mJy

{\bf 0954+346:} Confusing, steep-spectrum source at $09^{h}57^{m}48.^{s}3; 
+34^{o}17'28"$ (4.8 arc min away). $S_{1.4}\approx 90$ mJy

{\bf 0955+320:} Confusing, steep-spectrum source at $09^{h}58^{m}25.^{s}37; 
+31^{o}47'17"2$ (7.1 arc min away). $S_{1.4}\approx 170$ mJy

{\bf 1003+484:} 3C235. The spectrum breaks at about 320 MHz. $\alpha_{0.038}^{0.4}
\approx 0.82$, $\alpha_{0.4}^{15}\approx 1.16$

{\bf 1014+397:} The optical magnitudes are for the galaxy at 
$10^{h}17^{m}18.^{s}60; +39^{o}31'19"3$ (cross '1' in Paper II). Vigotti et al. 
(1989) identified this extended double source with another brighter galaxy at 
$10^{h}17^{m}17.^{s}86; +39^{o}31'46"5$. Thompson et al. (1992) determined it as 
a NLRG with the redshift of 0.089

{\bf 1017+487:} in Abell cluster 1003

{\bf 1049+384:} The optical spectrum shows intermediate properties between 
galaxies and quasars (Allington-Smith et al. 1988)

{\bf 1104+365:} The optical spectrum as above

%{\bf 1124+488:} An apparent cluster of 5--6 sources. VLA 1465-MHz A-array and 
%C-array maps by Machalski \& Condon (unpublished)

{\bf 1127+507:} Confusing  steep-spectrum source 1126+506 at $11^{h}29^{m}12.^{10}; 
+50^{o}23'35"$ (6.1 arc min away). $S_{1.4}\approx 348$ mJy

{\bf 1129+351:} The optical spectrum shows intermediate properties between 
galaxies and quasars (Allington-Smith et al. 1988)
 
{\bf 1131+493:} UGC6549;  IC708; in Abell cluster 1314. References to WSRT maps 
and  physical parameters in Condon \& Broderick (1988)

{\bf 1132+492:} IC711; in Abell cluster 1314. Low-resolution Effelsberg map at 
2.7 GHz in Haslam et al. (1978)

{\bf 1141+466:} in Abell clusted 1361. Low-resolution Effelsberg map at 2.7 GHz 
in Waldhausen et al. (1979). Confusing, flat-spectrum source at 
$11^{h}43^{m}10_{.}^{s}9; +46^{o}23'40"$ (5.5 arc min away). $S_{1.4}\approx 190$ 
mJy. For its low-resolution maps cf. Rudnick \& Owen (1977) and Andernach 
et al. (1980). 4885-MHz VLA map of central part of the source is shown in 
Figure A1 (Appendix)

{\bf 1144+352:} A total extent of the radio emission of about 10 arc min (about 
990 kpc) is suggested from the 4.85-GHz map N111200W of Condon et al. (1989). 
Its position angle $(PA)$ of about 105 deg is compatible with $PA=118^{o}$ of 
a two-sided, about 45 kpc extended, emission from the very compact and bright 
core on the map 11480+35071B of Becker et al. (1995). Moreover, the 
VLBI-scale structure (about 22 mas, corresponding to about 37 pc)  observed by 
Henstock et al. (1995), has $PA=121.^{o}5$

{\bf 1144+497:} Confusing source at $11^{h}47^{m}50.^{s}2$; $+49^{o}28'05"$ 
(4.1 arc min away). $S_{1.4}\approx 80$ mJy. Though the blue optical object 
lies on the overall axis of this double source, the identification is not 
convincing

{\bf 1151+384:} Bright, confusing, steep-spectrum double source 1151+383 at 
$11^{h}54^{m}01.^{s}2; +38^{o}05'07"$ (6.9 arc min away). 
$S_{1.4}\approx 500$ mJy

{\bf 1152+462:} Confusing source 1152+463 at $11^{h}54^{m}43.^{s}95$; 
$+46^{o}01'32"4$ (7.5 arc min away). $S_{1.4}=217\pm 10$ mJy 
Designated as 1152+462B in Paper V)

{\bf 1158+345:} The optical identification is not certain

{\bf 1202+499B:} Confusing source 1202+499A (3.0 arc min away).
$S_{1.4}=154$ mJy

{\bf 1216+475:} M106; NGC4258; UGC7353. Low-luminosity, starburst galaxy with 
a trace of non-thermal nucleus. References to WSRT and Effelsberg maps, as well 
as physical parameters in Condon \& Broderick (1988)

{\bf 1218+489:} Though the blue optical object lies on overall axis of this 
source (cf. Paper IV), the identification may be an accidental one

{\bf 1226+492:} Confusing, flat-spectrum source at $12^{h}28^{m}52.^{s}9$; 
$+49^{o}04'36"$ (6.6 arc min away). $S_{1.4}\approx 50$ mJy

{\bf 1230+486:} Very likely variable at frequencies above 5 GHz. Confusing 
steep-spectrum source at $12^{h}32^{m}35.^{s}7$; $+48^{o}16'50"$ (4.7 arc min 
away) identified with 4C48.35. $S_{1.4}\approx 150$ mJy

{\bf 1231+495:} Faint red optical object at $12^{h}34^{m}20.^{s}61$; 
$+49^{o}14'18"7$ (cf. Paper IV) might be associated with this double radio source

{\bf 1237+353:} Confusing, compact, steep-spectrum source at 
$12^{h}40^{m}19.^{s}2$; $+34^{o}56'39"$ (6.4 arc min away). $S_{1.4}\approx 
190$ mJy

{\bf 1239+328:} NGC4631; UGC7865. Low-luminosity star-burst galaxy. References 
to WSRT, NRAO interferometer, and Effelsberg maps, as well as physical 
parameters in Condon \& Broderick (1988)

{\bf 1248+350:} Deep observations of the field at 408 MHz (5C12 survey: Benn et 
al. 1982), at 610 and 1415 MHz (WSRT surveys: Katgert 1978; Katgert et al. 1973, 
respectively). Identified with 5C12.2 and 1248+35W1. Confusing, faint, double 
source (5C12.4; 1248+34W1) at $12^{h}50^{m}46.^{s}0; +34^{o}39'59"$ (4.7 
arc min away). $S_{1.4}\approx 90$ mJy

{\bf 1249+508:} 3C277. The spectrum breaks at about 1.1 GHz. 
$\alpha_{0.15}^{1.1}\approx 0.90$, $\alpha_{1.1}^{10}\approx 1.18$

{\bf 1256+489:} 4C48.36. Confusing, steep-spectrum source at 
$12^{h}59^{m}42.^{s}4; +48^{o}43'22"$ (5.4 arc min away). $S_{1.4}\approx 110$ 
mJy

%{\bf 1308+328:} 'New' compact, Gigahertz Peaked Spectrum (GPS) source, strongly 
%variable from the radio to X-ray, serendipitiously found during the research 
%(cf. Machalski \& Engels 1994)

{\bf 1322+366:} NGC5141; UGC8433. WSRT 5-GHz map in Fanti et al. (1977). 
Physical parameters in Condon \& Broderick (1988)

{\bf 1324+498A:} Confusing, flat-spectrum source 1324+498B at 
$13^{h}26^{m}39.^{s}3; +49^{o}33'55"$ (4.1 arc min away). $S_{1.4}\approx 90$ 
mJy

{\bf 1327+474:} M51; NGC5194; UGC8493. Low-luminosity star-burst galaxy with 
faint non-thermal radio core. References to WSRT and Effelsberg maps, as well as 
physical parameters in Condon \& Broderick (1988). The spectrum breaks at about 
1.4 GHz. $\alpha_{0.038}^{1.4}\approx 0.67$, $\alpha_{1.4}^{5}\approx 1.07$

{\bf 1329+503:} Confusing, steep-spectrum source at $13^{h}30^{m}56.^{s}4; 
+50^{o}09'04"$ (6.7 arc min away). $S_{1.4}\approx 200$ mJy

{\bf 1348+352:} Unique radio source; a more detailed discussion in the Appendix

{\bf 1354+325:} For a discussion of the optical field, cf. Machalski \& Condon (1985b)

{\bf 1413+349:} Confusing, steep-spectrum source at $14^{h}16^{m}17.^{s}2; 
+34^{o}48'05"$ (4.4 arc min away). $S_{1.4}\approx 130$ mJy

{\bf 1415+463:} 4C46.29. Confusing source 1414+463 at $14^{h}16^{m}42.^{s}9; 
+46^{o}03'04"$ (6.0 arc min away). $S_{1.4}\approx 140$ mJy

%{\bf 1432+382:} VLA 4885-MHz A-array data on the confusing sources by Machalski 
%(unpublished)

{\bf 1452+502A:} Close pair (2.5 arc min apart) with compact quasar 1452+502B. 
All flux densities in the surveys given in column 2 are strongly confused

{\bf 1504+346:} in Abell cluster 2025

{\bf 1507+476:} The optical galaxy is 2.1 arc sec apart from this compact radio 
source whose observed structure was deconvolved into two 'point' components 
separated by 0.87 arc sec (Paper III)

{\bf 1527+349:} For a discussion of the optical field cf. Paper III

{\bf 1546+487:} Confusing, steep-spectrum source at $15^{h}47^{m}40.^{s}4; 
+48^{o}39'22"$ (7.1 arc min away). $S_{1.4}\approx 220$ mJy

{\bf 1613+345:} Two confusing sources at $16^{h}15^{m}39.^{s}2$; $+34^{o}21'57"$ 
and $16^{h}15^{m}44.^{s}5$; $+34^{o}21'15"$ (4.8 and 6.1 arc min away, 
respectively), was recorded as 1613+344 in Owen et al. (1983) with a total flux 
$S_{1.4}\approx 70$ mJy

{\bf 1615+351:} NGC6109; UGC10316. References to WSRT maps, and physical 
parameters in Condon \& Broderick (1988)

{\bf 1626+396:} NGC6166; UGC10409. WSRT 1.4 and 5 GHz maps in Jaffe \& Perola 
(1974). Physical parameters in Condon \& Broderick (1988)

{\bf 1636+379:} in Abell cluster 2214



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