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Bull. Spec. Astrophys. Obs., 1998, 46, 28{61
Simultaneous spectra of complete sample of sources
from the PMN survey
M.G. Mingaliev a , A.M. Botashev a , V.A. Stolyarov a;b
a Special Astrophysical Observatory of the Russian AS, Nizhnij Arkhyz 357147, Russia
b Nuôeld Radio Astronomy Laboratories, Jodrell Bank, Maccleseld, Cheshire, SK11 9DL, UK
Received November 11, 1998; accepted November 25, 1998.
Abstract. In this report we present the results of observations of a complete sample of sources
from the PMN Survey. The adopted selection criteria were: ux density  200 mJy at the PMN
Survey frequency 4.8 GHz; 0 h RA24 h ; {21 ô Dec{17 ô ; jbj  10 ô to exclude the galactic plane.
Five runs of observations were accomplished in 1995{1996. The observations were made at 0.96,
2.3, 3.9, 7.7 and 11.2 GHz at the RATAN-600 radio telescope. For all sources of the sample, ux
densities at ve frequencies and their simultaneous spectra were determined, accuracies in RA
were improved 5{10 times. Identications with data from the Texas Survey were performed.
Key words: surveys { extragalactic sources { radio continuum
1. Introduction
Broad waveband spectra of radio sources including
high frequency data are desirable for a number of rea-
sons. Over the last decade researchers have identied
a new class of very high-redshift objects that are more
closely related to normal galaxies than to quasars.
Surveys with radio telescopes have been instrumen-
tal in nding these extremely distant galaxies, which
are barely visible at optical wavelengths. The selec-
tion of candidates with steep radio spectra has proved
to be a particular eective means for nding galaxies
with redshifts greater than 2. On the other hand, they
uncover at spectrum sources which are likely to be
compact and useful as radio astrometric standards as
well as candidates for further interferometric observa-
tions. Third, they provide information about physics
and, in particular, about the high-energy particles re-
sponsible for radio emission. And last but not least,
simultaneous observations at several wavelengths will
exclude variability of sources in interpretation of their
spectra.
This paper continues the series of articles devoted
to the research of complete samples of sources from
dierent radio catalogues (see, e.g. Mingaliev and
Khabrakhmanov, 1995) at the RATAN-600 radio tele-
scope. Here we present the results of investigation of
a complete sample of radio sources from the PMN
Survey (Griôth et al., 1994).
2. Observations
The adopted selection criteria of the complete sample
from the PMN Survey (Griôth et al., 1994) were as
follows:
 ux density S  200 mJy at the PMN Survey
frequency (4.8 GHz);
 00 h  RA 24 h ;
 21 ô  Dec 17 ô ;
 galactic latitude jbj 10 ô to exclude the
galactic plane.
A total of 262 objects have been selected.
The observations were made in the frequency
bands 0.96, 2.3, 3.9, 7.7 and 11.2 GHz using a com-
plex of broad-band radiometers of the RATAN-600
(Nizhel'skij, 1995; Berlin, 1997). The observations
were conducted with the North sector of the tele-
scope in a transit mode during several runs in 1995{
1996. The gain of the receivers was controlled by the
reference noise generator during each passage of the
source. Each source was observed 5{8 times. Unfor-
tunately, because of bad weather conditions and mal-
function of the receivers, ve sources from the sample
were not observed. As a ux density and coordinate
standard we used the strong radio source 1245-197
(RA 1950:0 = 12 h 45 m 45: s 22, Dec 1950:0 = {19 ô 42 0
57: 00 5).
The adopted ux densities are listed in Table 1.
c
Special Astrophysical Observatory of the Russian AS, 2000

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 29
Table 1: The ux densities for the reference source
1245-197
Frequency, GHz 11.2 7.7 3.9 2.3 0.96
Flux density, Jy 1.24 1.75 3.0 4.0 6.3
3. Data reduction
3.1. Right ascension measuring
A dierential method used for measuring RA in com-
bination with the xed focus mode (Soboleva et al.,
1986) excluded completely the pointing error. The ob-
servations at 3.9 GHz (=7.6 cm) were used for these
purposes because, according to formula (1) and tak-
ing into account the sensitivity of the radiometer, ob-
servations at this wavelength had the best coordinate
accuracy:
n = 1
2

Tn
T s
 0:5 ; (1)
where
n | uctuation sensitivity of the radio telescope;
T c | antenna temperature of the observed source;
 0:5 | full width at half maximum (FWHM).
The exact time of passage of a source across the
beam and the antenna temperature were determined
for each source using the optimum automatic tting
of the gaussian into the drift scan of the source with
the help of the \FGR" data reduction programme
(Verkhodanov, 1995). The next step was the deter-
mination of the average crossing times. The measure-
ment errors were dened as standard deviations. One
can nd the achieved accuracy for each source in Ta-
ble 2. A more detailed description of the methods
and the accuracy of coordinate measurements on the
radio telescope can be found in (Mingaliev and Cher-
nenkov, 1991).
3.2. Flux density measurement
The ux density was determined as an average value
over 8 observations, and the error as a standard
deviation. The accuracy of a single measurement is
found from the sum of errors of
{ gaussian tting of the passage curve (in general, it
is determined from signal-to-noise ratio;
{ statistics of antenna setting from one observation
to another;
{ gain and calibration signal stability.
The accuracy of ux density measurements at
11.2, 7.7 and 3.9 GHz was mostly aected by re-
ceiver's noises and statistics of antenna settings; so
the accuracy at the best sensitivity band, 3.9 GHz, is
in general 2{3% or better. The accuracy at 2.3 and
0.96 GHz was impaired by strong interferences from
­3 ­2 ­1 0 1 2 3 4
0
20
40
60
DRA, sec
Number
of
sources,
N
­10 ­8 ­6 ­4 ­2 0 2 4 6 8 10
0
10
20
30
40
DRA/s
Number
of
sources,
N
Figure 1: The distribution of
RA and
RA= for
the PMN survey. The parameters of the gaussian
curve (on the upper histogram) are M = 0:081 s,
sd = 0:864 s.
traôc, satellites and military radar systems, atmo-
spheric electricity.
The results of ux measurements for every source
( ux densities and their errors) are listed in Ta-
ble 3. The technique of ux measurements with the
RATAN-600 broad-band radiometers is described in
more detail by Mingaliev et al. (1978) and Aliakberov
et al. (1985).
4. Results
Thanks to good sensitivity and resolving power in RA
at 7.6 cm we have improved the RA of these sources
too. These results will be helpful in further optical
identications. For most sources (70%) the accu-
racy in RA is equal to or better than 0: s 1, for the
rest of them it is better than 0: s 2. The RA deter-
mined in the framework of this programme were com-
pared with positions from the PMN ( c =4.85GHz)
and Texas (interferometric survey with high an-
gular resolution and multibeam shape of the dia-
gram,  c =0.365GHz, see Douglus, 1980) surveys. In
Fig. 1(a,b) one can see the histograms of the residuals

RA = RARATAN RAPMN (2)

30 MINGALIEV, BOTASHEV, STOLYAROV
­1.0 ­0.5 0.0 0.5 1.0
0
10
20
30
40
DRA, sec
Number
of
sources,
N
­20 ­10 0 10 20
0
20
40
DRA/s
Number
of
sources,
N
Figure 2: The distribution of
RA and
RA= for
the Texas survey. The parameters of the gaussian
curve (upper panel) are M = 0:038 s, sd = 0:156 s.
and the residuals normalized to the standard sum of
the quoted rms errors

RA
 = (RARATAN RAPMN ) 2
( 2
RATAN +  2
PMN ) 1=2
(3)
and in Fig. 2(a,b) the same distributions for the Texas
catalogue. The distribution of the residuals
RA is
gaussian in both cases.
The improved values of coordinates which are pos-
sible to use in further identications are listed in Ta-
ble 2. Column 1 gives the names of the sources accord-
ing to the PMN catalogue; columns 2 and 3 contain
RA 2000 and its error for each source from our obser-
vations; column 4 is Dec 2000 of the sources according
to the PMN survey.
The results of ux density measurements are listed
in Table 3 and the spectra of the sources are shown
in Fig. 4. In order to derive additional information
about the variability of the sources, we have added
the ux densities from the Texas Sky Survey at the
frequency 0.365 GHz and of the PMN catalogue at
4.85 GHz to the spectra of the sources. A comparison
between the sources of our list (after improving the
RA in the course of our observations) and the Texas
Survey has revealed a match for 80% of the sources.
Table 3 presents the followings:
#### ### ### ### ### ### ###
#
##
##
##
6SHFWUDO#LQGH[##a ##########
1XPEHU#RI#VRXUFHV##1
#### #### ### ### ### ### ###
#
##
##
##
6SHFWUDO#LQGH[##a ###########
1XPEHU#RI#VRXUFHV##1
Figure 3: The distribution of two-frequency spectral
indices  11:2=3:9 between 11.2 and 3.9 GHz (upper
panel) and  3:9=0:365 between 3.9 and 0.365 GHz
(lower panel).
column 1: the source name according to the PMN
notation (J2000.0);
column 2: the number of the run of observations,
where 1 is July 1995, 2 is August 1995, 3 is December
1995, 4 and 5 are January and October 1996, respec-
tively;
columns 3{16: the ux density in mJy and its stan-
dard error at 11.2, 7.7, 4.85 (PMN), 3.9, 2.3, 0.96,
and 0.365 GHz (Texas), respectively;
column 17: the two-frequency spectral index
 11:2=3:9 , computed from the formula
 = log(S( 1 )=S( 2 ))=log( 1 = 2 )
for the uxes at 11.2 and 3.9 GHz;
column 18: the spectral index  3:9=0:365 (if there is
no counterpart in the Texas catalogue, the spectral
index  3:9=0:96 is used instead).
One can see the two-frequency spectral index dis-
tribution in the bands of 11.2{3.9 GHz and 3.9{
0.365(0.96) GHz in Fig. 3(a,b).
5. Conclusions
For 262 radio sources from the PMN Tropical Survey
the following has been done:

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 31
{ the ux densities in the 11.2, 7.7, 3.9, 2.3 and
0.96 GHz frequency bands have been measured;
{ simultaneous spectra in the 11.2 { 0.96 GHz bands
have been determined;
{ the accuracy in RA has been improved by a factor
of 5{7.
Making further steps in the accomplishment of
this research programme, the following is supposed
to be done: optical identication of the PMN sources
with the Digitized Sky Survey (Lasker et al., 1990),
identication in other wavebands, selection of vari-
able sources with the help of the simultaneous spec-
tra taken in the course of fullment of this programme
and data obtained with other telescopes for dierent
epochs.
Acknowledgements. This research is partially sup-
ported by the Russian Foundation for Basic Research
project No. 95-02-04972, and INTAS project No. 94-4010.
References
Aliakberov K.D., Mingaliev M.G., Naugol'naya M.N.,
Trushkin S.A., Sharipova L.M., Yusupova S.N., 1985,
Astroz. Issled. (Izv.SAO), 19, 60
Berlin A.B., Maksyasheva A.A., Nizhel'skij N.A.,
Pilipenko A.M., Tsybulev P.G., 1997, Proceed. of 27-
th Radio Astron. Conf., St.Petersburg, 115
Douglus J.N., 1980, The University of Texas Publications
in Astronomy, No. 17
Griôth M.R., Wright A.E., Burke B.F., and Ekers R.D.,
1994, Astrophys. J. Suppl. Ser., 90, 179
Lasker B.M., Sturch C.R., McLean B.J., Russell J.L.,
Jenkner H., and Shara M., 1990, Astron. J., 99, 2019
Lipovka N.M., Stotskij A.A., 1972, Bull. GAO, 188, 238
Mingaliev M.G. and Chernenkov V.N., 1991, As-
troz. Issled. (Izv.SAO), 31, 153
Mingaliev M.G. and Khabrakhmanov A.R., 1995, Pis'ma
Astron. Zh., 72, 12
Mingaliev M.G., Pustil'nik S.A., Trushkin S.A., Ki-
rakosyan R.M., Malumyan V.G., 1978, Astrozika, 14,
91
Nizhel'skij N.A., 1996, SAO Annual Report, 57
Soboleva N.S., Temirova A.V., Pyatunina T.B., 1986,
Prepr. SAO USSRAS, No. 32L, 22
Verkhodanov O.V., 1995, Prepr. SAO RAS, No. 106, 57

32 MINGALIEV, BOTASHEV, STOLYAROV
Table 2: The coordinates for the complete sample of
sources
Object name RA 2000 RMS, sec Dec 2000
0001-1741 00:01:06.52 0.089 -17:41:31.8
0003-1727 00:03:21.83 0.02 -17:27:12.1
0003-1941 00:03:15.81 0.15 -19:41:49.9
0008-1939 00:08:18.25 0.21 -19:39:36.8
0009-2056 00:09:05.91 0.15 -20:56:11.7
0015-1807 00:15:34.30 0.14 -18:07:14.0
0015-1812 00:15:02.05 0.07 -18:12:51.0
0015-1929 00:15:59.99 0.09 -19:29:10.6
0020-2014 00:20:26.21 0.16 -20:14:50.9
0021-1910 00:21:12.97 0.073 -19:10:38.0
0026-2004 00:26:13.96 0.057 -20:04:54.9
0034-1759 00:34:24.14 0.18 -17:59:31.2
0035-2004 00:35:08.83 0.029 -20:04:01.2
0039-1854 00:39:16.95 0.243 -18:54:09.5
0040-2043 00:40:48.25 0.053 -20:43:41.2
0054-1952 00:54:32.94 0.065 -19:52:47.9
0059-1700 00:59:06.80 0.028 -17:00:38.2
0100-1749 01:00:10.19 0.062 -17:48:59.5
0116-2052 01:16:51.38 0.035 -20:52:09.9
0118-1849 01:18:34.19 0.034 -18:49:13.9
0119-1940 01:19:08.64 0.074 -19:40:05.8
0135-2008 01:35:37.56 0.041 -20:08:47.7
0140-1729 01:40:23.22 0.05 -17:29:29.9
0142-1714 01:42:23.56 0.22 -17:14:10.9
0151-1732 01:51:06.00 0.118 -17:32:44.1
0202-1948 02:02:14.07 0.058 -19:48:13.7
0204-1701 02:04:57.86 0.031 -17:01:19.8
0205-1801 02:05:19.84 0.20 -18:01:13.0
0219-1842 02:19:21.47 0.062 -18:42:41.1
0227-1713 02:27:06.22 0.072 -17:13:19.2
0231-2040 02:31:35.99 0.099 -20:40:26.3
0237-1932 02:37:43.97 0.089 -19:32:22.2
0248-2002 02:49:00.94 0.146 -20:02:34.2
0249-1928 02:49:00.47 0.05 -19:28:46.2
0255-2027 02:55:54.81 0.21 -20:27:44.6
0307-1748 03:07:55.83 0.25 -17:48:08.7
0320-1702 03:20:19.04 0.07 -17:02:36.0
0325-1802 03:25:53.31 0.049 -18:02:00.3
0335-1832 03:35:05.00 0.075 -18:32:28.5
0354-1755 03:54:20.63 0.072 -17:55:02.1
0405-1831 04:05:56.27 0.029 -18:31:04.9
0409-1757 04:09:06.72 0.028 -17:57:06.5
0415-2022 04:15:08.24 0.23 -20:22:18.8
0416-1851 04:16:36.54 0.064 -18:51:00.5
0416-2056 04:16:04.27 0.047 -20:56:21.3
0425-1700 04:25:28.75 0.19 -17:00:19.1
0431-1704 04:31:58.55 0.086 -17:04:02.1
0437-1844 04:37:01.49 0.16 -18:44:53.2
0438-2012 04:38:50.65 0.045 -20:12:25.9
0444-1822 04:44:57.17 0.109 -18:22:36.8
0444-2051 04:44:09.64 0.03 -20:51:01.1
0448-2032 04:48:30.54 0.21 -20:32:06.3
0450-1837 04:50:35.93 0.026 -18:37:10.7
0451-1730 04:51:18.40 0.24 -17:30:16.3
0455-2034 04:55:23.51 0.097 -20:34:18.5
0501-1706 05:01:42.89 0.029 -17:06:11.9
0514-1957 05:14:52.72 0.064 -19:57:36.4
0514-2029 05:14:17.34 0.08 -20:29:21.7
0517-1756 05:17:23.95 0.23 -17:56:12.0
0521-1737 05:21:23.67 0.071 -17:37:27.5
Table 2: The coordinates for the complete sample of
sources (continue)
Object name RA 2000 RMS, sec Dec 2000
0521-2047 05:21:39.07 0.022 -20:47:34.0
0525-2010 05:25:27.92 0.043 -20:10:54.3
0546-1725 05:46:17.76 0.044 -17:25:52.3
0547-1958 05:47:55.04 0.065 -19:58:06.2
0553-1709 05:53:51.44 0.039 -17:09:57.6
0559-1817 05:59:46.28 0.042 -18:17:29.2
0603-1716 06:03:57.76 0.038 -17:16:16.8
0605-1755 06:05:57.72 0.069 -17:55:15.3
0606-2022 06:06:33.62 0.026 -20:22:01.7
0610-1847 06:10:17.78 0.15 -18:47:49.0
0617-1715 06:17:33.51 0.079 -17:15:15.4
0618-2051 06:18:27.78 0.042 -20:51:51.7
0619-2054 06:19:37.22 0.046 -20:54:13.6
0621-1715 06:21:01.55 0.058 -17:15:52.0
0623-1708 06:23:07.30 0.059 -17:08:26.0
0629-1959 06:29:23.87 0.085 -19:59:18.4
0633-1802 06:33:09.94 0.035 -18:02:50.4
0636-2031 06:36:32.06 0.07 -20:31:14.7
0636-2041 06:36:31.92 0.04 -20:41:54.0
0824-1827 08:24:03.93 0.16 -18:27:44.5
0828-1952 08:28:02.85 0.089 -19:52:33.0
0836-2017 08:36:39.11 0.027 -20:17:05.5
0837-1951 08:37:11.01 0.044 -19:51:53.5
0844-1846 08:44:58.27 0.25 -18:46:06.1
0847-1755 08:47:11.10 0.093 -17:55:02.1
0847-2057 08:47:05.20 0.071 -20:57:49.4
0852-2047 08:53:00.25 0.106 -20:47:21.7
0858-1950 08:58:05.23 0.103 -19:50:34.3
0859-1922 08:59:38.71 0.06 -19:22:25.1
0902-1721 09:03:00.06 0.22 -17:21:05.2
0904-1957 09:04:41.16 0.225 -19:57:36.0
0906-2019 09:06:51.23 0.048 -20:19:57.4
0907-2026 09:07:54.51 0.109 -20:26:54.0
0909-1808 09:09:45.10 0.046 -18:08:36.9
0914-1842 09:14:27.70 0.11 -18:42:52.9
0927-2034 09:27:51.91 0.045 -20:34:51.4
0929-1820 09:29:02.26 0.31 -18:20:35.6
0931-1830 09:31:22.98 0.098 -18:30:14.2
0932-2017 09:32:46.04 0.06 -20:17:59.2
0935-1939 09:35:15.91 0.075 -19:39:10.1
0939-1731 09:39:19.17 0.19 -17:31:47.0
0945-1953 09:45:17.11 0.21 -19:53:27.3
0946-2020 09:46:50.55 0.064 -20:20:48.4
0948-1828 09:48:43.19 0.196 -18:28:32.2
0953-1947 09:53:47.21 0.06 -19:47:38.1
1006-1743 10:06:18.45 0.065 -17:43:10.1
1017-2016 10:17:10.11 0.17 -20:16:36.2
1020-1924 10:20:48.33 0.091 -19:24:51.9
1023-1933 10:23:18.26 0.088 -19:33:41.5
1024-1838 10:24:45.96 0.033 -18:38:31.2
1028-2027 10:28:59.25 0.046 -20:27:33.8
1029-1852 10:29:33.05 0.037 -18:52:43.1
1035-2011 10:35:02.27 0.07 -20:11:30.1
1036-1955 10:36:40.51 0.114 -19:55:50.0
1040-1924 10:40:57.21 0.053 -19:24:05.6
1048-1909 10:48:06.73 0.03 -19:09:25.1
1051-2023 10:51:32.22 0.027 -20:23:41.7
1052-1845 10:52:34.60 0.054 -18:45:11.3
1105-1851 11:05:24.63 0.063 -18:51:37.7
1110-1858 11:10:00.24 0.068 -18:58:49.4

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 33
Table 2: The coordinates for the complete sample of
sources (continue)
Object name RA 2000 RMS, sec Dec 2000
1127-1857 11:27:04.21 0.14 -18:57:10.2
1133-1954 11:33:36.82 0.117 -19:54:10.3
1134-1727 11:34:23.56 0.104 -17:27:48.4
1136-1733 11:36:03.15 0.038 -17:33:02.6
1144-1741 11:44:26.81 0.104 -17:41:22.3
1149-1943 11:49:56.31 0.16 -19:43:47.0
1150-1930 11:50:31.22 0.244 -19:30:34.2
1151-1723 11:51:03.11 0.102 -17:23:59.0
1153-1816 11:53:32.64 0.075 -18:16:12.2
1155-1804 11:55:29.32 0.13 -18:04:41.1
1201-1852 12:01:53.90 0.099 -18:52:29.2
1209-2032 12:09:14.65 0.06 -20:32:34.1
1211-1926 12:11:57.92 0.027 -19:26:01.3
1215-1731 12:15:46.72 0.038 -17:31:41.6
1240-1717 12:40:25.75 0.042 -17:17:18.6
1243-1833 12:43:35.63 0.087 -18:33:50.6
1249-2055 12:49:21.33 0.118 -20:55:18.8
1251-1717 12:51:14.48 0.21 -17:17:01.1
1254-1845 12:54:11.73 0.136 -18:45:29.1
1258-1750 12:58:55.22 0.252 -17:50:27.9
1258-1759 12:58:38.07 0.071 -17:59:58.9
1301-2020 13:01:52.61 0.17 -20:20:41.6
1304-1932 13:04:33.69 0.042 -19:32:46.1
1306-1719 13:06:32.69 0.16 -17:19:14.5
1312-2027 13:12:08.00 0.049 -20:27:03.7
1315-1858 13:15:05.46 0.092 -18:58:20.6
1330-2056 13:30:07.50 0.053 -20:56:15.0
1337-1811 13:37:37.50 0.039 -18:11:34.1
1342-2051 13:42:04.56 0.089 -20:51:19.5
1343-1748 13:43:37.36 0.061 -17:48:05.0
1344-1723 13:44:14.36 0.094 -17:23:40.9
1356-1724 13:56:06.96 0.23 -17:24:37.6
1356-1751 13:56:53.12 0.224 -17:51:51.4
1357-1744 13:57:05.47 0.184 -17:44:02.4
1402-1840 14:02:48.33 0.074 -18:40:43.4
1413-2020 14:13:35.02 0.18 -20:20:32.7
1416-1705 14:16:34.47 0.121 -17:05:40.3
1419-1928 14:19:49.73 0.079 -19:28:20.9
1421-1931 14:21:28.76 0.21 -19:31:40.1
1423-1816 14:23:36.04 0.072 -18:16:09.5
1425-1756 14:25:57.85 0.05 -17:56:44.1
1432-1801 14:32:57.61 0.059 -18:01:29.9
1454-1925 14:54:23.46 0.086 -19:25:01.9
1455-1700 14:55:02.72 0.085 -17:00:15.9
1515-1939 15:15:40.37 0.13 -19:39:54.0
1525-1903 15:25:12.45 0.21 -19:02:59.7
1530-2013 15:30:17.23 0.062 -20:13:41.4
1542-1803 15:42:04.58 0.151 -18:03:43.3
1551-1754 15:51:14.38 0.047 -17:54:58.1
1605-1734 16:05:01.99 0.07 -17:34:13.7
1607-2039 16:07:57.25 0.29 -20:39:36.1
1616-1723 16:16:59.82 0.064 -17:23:21.0
1619-1817 16:19:16.56 0.22 -18:17:23.5
1642-2006 16:42:03.27 0.28 -20:06:58.0
1644-1804 16:44:35.61 0.096 -18:04:29.6
1647-1926 16:47:53.78 0.06 -19:26:31.5
1657-2004 16:57:33.24 0.19 -20:04:42.0
1658-2011 16:58:04.71 0.072 -20:11:38.3
1701-1903 17:01:26.64 0.15 -19:03:38.8
1702-1758 17:02:38.24 0.035 -17:58:07.3
Table 2: The coordinates for the complete sample of
sources (continue)
Object name RA 2000 RMS, sec Dec 2000
1703-2031 17:03:16.77 0.105 -20:31:36.1
1709-1728 17:09:34.15 0.042 -17:28:55.0
1710-2030 17:10:09.73 0.113 -20:30:25.9
1712-1819 17:12:31.56 0.11 -18:19:54.9
1911-1712 19:11:40.75 0.029 -17:12:05.6
1911-1908 19:11:29.65 0.097 -19:08:27.0
1911-1921 19:11:56.40 0.129 -19:21:57.7
1911-2006 19:11:09.56 0.099 -20:06:55.4
1917-1921 19:17:44.79 0.064 -19:21:38.2
1925-1836 19:25:59.22 0.116 -18:36:55.1
1932-1931 19:32:07.14 0.025 -19:31:46.8
1936-1711 19:36:13.39 0.27 -17:11:22.8
1938-1749 19:38:04.93 0.057 -17:49:24.2
1948-1857 19:48:47.69 0.21 -18:57:37.3
1949-1957 19:49:53.45 0.023 -19:57:16.9
1952-1936 19:52:43.84 0.102 -19:36:22.9
1955-1925 19:55:15.11 0.062 -19:25:49.1
2000-1748 20:00:56.92 0.025 -17:48:56.2
2000-1921 20:00:08.54 0.028 -19:21:41.8
2005-1822 20:05:17.14 0.03 -18:22:01.8
2015-1703 20:15:57.66 0.103 -17:03:18.7
2022-2007 20:22:18.00 0.087 -20:07:05.0
2022-2058 20:22:59.31 0.26 -20:58:04.7
2023-1911 20:23:36.11 0.23 -19:11:38.2
2030-1702 20:30:29.90 0.22 -17:02:06.6
2035-1745 20:35:34.04 0.22 -17:45:21.9
2038-2011 20:38:29.38 0.099 -20:11:09.3
2047-1821 20:47:16.80 0.17 -18:21:16.3
2053-1838 20:53:19.00 0.08 -18:38:37.6
2056-1956 20:56:04.25 0.025 -19:56:31.6
2101-1747 21:01:43.28 0.19 -17:47:58.1
2114-1819 21:14:17.41 0.125 -18:19:01.4
2116-2055 21:16:36.17 0.021 -20:55:45.7
2129-1821 21:29:21.36 0.039 -18:21:16.4
2135-1734 21:35:16.90 0.049 -17:34:24.6
2137-2042 21:37:49.91 0.039 -20:42:36.8
2138-1810 21:38:41.86 0.043 -18:10:35.8
2138-1843 21:38:04.99 0.031 -18:43:28.8
2139-1838 21:39:39.42 0.048 -18:38:03.7
2147-1740 21:47:03.22 0.039 -17:40:11.5
2148-1723 21:48:36.70 0.027 -17:23:45.3
2149-1859 21:49:58.62 0.27 -18:59:27.8
2149-1912 21:49:41.84 0.22 -19:12:29.9
2151-1946 21:51:51.05 0.072 -19:46:07.9
2156-1813 21:56:57.22 0.039 -18:13:53.7
2157-1807 21:57:28.86 0.038 -18:07:01.6
2206-1800 22:06:55.11 0.27 -18:00:33.3
2206-1835 22:06:10.42 0.036 -18:35:34.1
2214-1701 22:14:25.62 0.034 -17:01:51.4
2233-2024 22:33:25.30 0.123 -20:24:57.0
2234-2055 22:34:56.99 0.05 -20:55:07.9
2235-1826 22:35:56.12 0.28 -18:26:16.4
2236-1706 22:36:09.68 0.23 -17:06:27.3
2237-1712 22:37:37.23 0.03 -17:12:45.5
2239-1720 22:39:10.70 0.063 -17:20:52.2
2245-1737 22:45:59.09 0.25 -17:37:20.4
2251-1848 22:51:31.16 0.07 -18:48:04.1
2252-2047 22:52:28.65 0.28 -20:47:23.2
2256-2011 22:56:41.21 0.16 -20:11:41.2

34 MINGALIEV, BOTASHEV, STOLYAROV
Table 2: The coordinates for the complete sample of sources (continued)
Object name RA 2000 RMS, sec Dec 2000
2257-1828 22:57:32.28 0.29 -18:28:44.2
2303-1841 23:03:02.90 0.042 -18:41:20.6
2304-1939 23:04:39.19 0.077 -19:39:25.4
2315-1800 23:15:48.06 0.027 -18:00:44.8
2320-1919 23:20:49.79 0.023 -19:19:17.3
2329-1923 23:29:33.69 0.045 -19:23:13.2
2330-1808 23:30:03.24 0.146 -18:08:04.8
2337-1752 23:37:56.43 0.064 -17:52:23.6
2347-1856 23:47:08.59 0.046 -18:56:31.2
2355-1810 23:55:55.46 0.19 -18:10:07.1
2357-1817 23:57:07.80 0.072 -18:17:44.1
2359-2048 23:59:19.71 0.063 -20:48:04.3
Table 3: The uxes for the complete sample of sources
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
0001-1741 3 89 13 124 19 205 15 250 11 347 17 801 42 989 104 0.98 0.58
0003-1727 5 474 11 684 21 894 48 1148 20 1578 60 3139 79 6764 134 0.84 0.75
0003-1941 1 140 10 { { 229 16 292 9 332 24 248 25 { { 0.70 -0.12
0008-1939 5 44 2 81 4 241 16 198 10 296 15 832 83 887 76 1.42 0.63
0009-2056 2 114 6 { { 204 15 273 7 414 21 833 83 1203 120 0.83 0.63
5 91 5 116 6 204 15 255 13 406 20 718 72 1203 35 0.98 0.66
0015-1807 5 129 6 190 10 251 17 293 15 328 16 388 39 306 30 0.78 0.02
0015-1812 3 331 24 341 17 324 20 417 7 378 19 344 25 306 30 0.22 -0.13
5 { { { { 324 20 323 16 314 16 292 29 306 30 - -0.02
0015-1929 1 101 8 { { 306 19 347 11 584 30 1208 121 2353 86 1.17 0.81
0020-2014 5 73 4 116 6 270 18 246 12 618 31 1611 120 { { 1.16 1.34
0021-1910 2 110 6 { { 456 26 421 6 635 32 1302 130 3231 132 1.27 0.86
5 118 6 139 7 456 26 467 10 629 32 1542 67 3231 131 1.30 0.82
0026-2004 1 119 9 { { 390 23 452 12 732 38 2058 103 3520 64 1.27 0.87
0034-1759 3 74 11 115 17 243 16 245 12 400 20 838 44 { { 1.13 0.88
0035-2004 1 196 14 { { 513 29 650 11 1163 60 780 78 7070 147 1.14 1.01
5 170 9 302 15 513 29 715 14 1241 43 3011 45 7070 147 1.36 0.97
0039-1854 5 165 8 159 8 225 16 266 15 222 11 262 26 { { 0.45 -0.01
0040-2043 2 235 12 { { 338 20 403 15 417 21 688 69 1264 36 0.51 0.48
5 191 10 259 13 338 20 395 9 482 24 681 68 1264 35 0.69 0.49
0054-1952 2 299 15 { { 276 18 285 10 235 12 288 29 580 74 -0.05 0.30
1 237 17 { { 276 18 234 8 297 21 358 36 580 73 -0.01 0.38
5 201 10 244 12 276 18 299 10 281 14 393 39 580 73 0.38 0.28
0059-1700 3 108 16 208 21 415 24 565 6 1032 9 2534 85 6932 118 1.57 1.06
0100-1749 5 155 8 226 11 419 24 555 10 781 27 1789 26 3889 131 1.21 0.82
0116-2052 1 518 32 { { 1415 74 1652 24 2701 40 5706 285 10616 172 1.10 0.79
5 556 18 814 19 1415 74 1774 11 2690 60 5677 45 10616 172 1.10 0.76
0118-1849 3 370 20 425 22 467 26 677 6 825 25 1486 63 2998 125 0.57 0.63
0119-1940 2 117 6 { { 242 16 212 22 299 15 513 51 1067 37 0.56 0.68
5 127 6 155 8 242 16 281 10 317 16 583 58 1067 37 0.75 0.56
0135-2008 2 572 29 { { 715 40 786 11 662 33 660 66 875 70 0.30 0.05
1 532 20 { { 715 39 780 18 676 35 576 58 875 69 0.36 0.05
5 567 12 684 16 715 39 833 14 739 27 734 21 875 69 0.36 0.02
0140-1729 5 60 3 98 5 295 19 321 9 420 11 934 27 1683 88 1.59 0.70
0142-1714 3 95 14 91 14 209 15 198 10 193 14 580 30 { { 0.70 0.77
0151-1732 5 397 17 429 21 340 21 318 12 191 10 143 20 { { -0.21 -0.57
0202-1948 2 275 14 { { 224 16 358 8 335 17 { { { { 0.25 -
1 288 15 { { 224 16 370 11 317 23 534 53 { { 0.24 0.26
5 190 10 235 12 224 16 331 10 306 15 201 20 { { 0.52 -0.35
0204-1701 3 1286 37 1207 18 1350 71 1508 11 1355 15 1261 54 1248 65 0.15 -0.08
0205-1801 5 { { { { 316 20 247 12 377 19 1052 105 { { - 1.03
0219-1842 3 379 19 315 16 258 17 360 5 306 15 577 41 { { -0.05 0.34
5 314 16 273 14 258 17 346 15 243 12 519 52 { { 0.09 0.29
0227-1713 5 103 5 232 12 353 21 428 19 597 30 1410 26 2877 45 1.35 0.80
0231-2040 1 88 6 { { 526 29 354 11 625 32 1385 139 1772 46 1.32 0.68

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 35
Table 3: The uxes for the complete sample of sources (continue)
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
5 100 5 124 6 526 29 342 7 574 29 1439 19 1772 46 1.17 0.69
0237-1932 2 372 19 { { 1314 70 1576 3 2964 148 6489 649 14419 434 1.37 0.93
0248-2002 1 88 6 { { 243 16 307 10 439 23 1166 117 1772 46 1.18 0.74
5 79 15 145 9 243 16 343 7 442 17 1344 23 1772 46 1.39 0.69
0249-1928 3 88 13 132 20 287 18 346 4 514 15 1182 50 2154 91 1.30 0.77
0255-2027 5 61 3 116 6 317 20 236 12 546 27 1577 51 { { 1.29 1.35
0307-1748 3 { { 47 9 204 15 170 9 329 16 743 39 1640 58 - 0.96
5 { { 55 3 204 15 151 8 325 16 787 22 1640 58 - 1.01
0320-1702 5 208 10 333 10 387 23 544 34 692 45 1350 24 2442 43 0.91 0.63
0325-1802 3 129 13 150 15 231 16 288 5 360 18 551 39 900 29 0.76 0.48
5 131 7 124 6 231 16 250 13 346 17 609 23 900 29 0.61 0.54
0335-1832 5 62 3 131 7 268 17 296 7 466 23 1241 25 2351 60 1.48 0.87
0354-1755 3 153 16 161 16 236 16 264 7 373 19 601 43 1286 79 0.52 0.67
0405-1831 4 145 4 163 4 273 9 301 4 405 10 715 36 980 54 0.69 0.50
5 135 7 211 11 273 18 308 8 323 16 865 68 980 54 0.78 0.49
0406-1749 5 298 11 387 14 444 25 517 8 561 28 612 61 295 26 0.52 -0.24
0409-1757 3 411 30 504 13 861 46 1048 10 1571 27 3054 55 5656 149 0.89 0.71
0415-2022 1 115 8 { { 245 17 258 8 533 27 1045 105 965 42 0.76 0.56
0416-1851 5 1124 25 1178 18 770 41 1180 31 1138 43 1329 130 679 36 0.05 -0.23
0416-2056 2 1339 67 { { 1293 68 1610 10 1887 94 3644 364 7589 136 0.17 0.65
0425-1700 3 96 15 102 15 318 20 253 10 482 15 1152 49 1821 87 0.92 0.83
5 87 4 118 6 318 20 299 15 417 21 1207 34 1821 87 1.17 0.76
0431-1704 5 56 3 150 8 307 19 344 10 495 25 1367 36 1990 92 1.72 0.74
0437-1844 3 902 29 940 16 1089 58 1124 17 { { 399 29 { { 0.21 -0.74
0438-2012 1 211 15 { { 286 18 368 13 376 27 688 69 965 42 0.53 0.41
5 202 10 263 13 286 18 360 6 355 18 680 19 965 42 0.55 0.42
0444-1822 5 73 4 89 5 243 16 276 9 412 21 817 23 1715 78 1.27 0.77
0444-2051 2 142 7 { { 225 16 300 7 425 21 990 99 1324 199 0.71 0.63
0448-2032 1 62 5 { { 217 15 263 9 458 24 { { 1091 77 1.36 0.60
0450-1837 3 261 19 356 18 427 25 524 8 462 14 222 22 349 39 0.66 -0.17
0451-1730 5 { { 65 3 382 22 194 10 437 22 1040 33 742 65 - 0.57
0455-2034 1 822 24 { { 1978 99 2278 36 3207 52 { { 11109 264 0.97 0.67
0501-1706 3 218 16 280 14 435 25 520 5 711 21 831 43 666 32 0.82 0.10
5 214 11 310 16 435 25 552 10 682 27 1056 88 666 32 0.90 0.08
0514-1957 5 88 4 96 5 209 15 193 6 283 14 592 59 773 70 0.75 0.59
0514-2029 1 407 16 { { 431 25 433 14 364 26 488 49 635 32 0.06 0.16
0517-1756 3 174 18 175 18 207 15 240 10 190 29 369 37 { { 0.30 0.31
0521-1737 5 238 12 329 16 470 27 400 19 452 23 587 59 657 33 0.49 0.21
0521-2047 2 134 7 { { 397 24 606 5 1061 53 2667 267 7401 200 1.43 1.06
5 89 5 302 13 397 23 619 9 1158 53 2836 62 7401 99 1.84 1.05
0525-2010 1 106 8 { { 219 15 182 6 210 15 394 39 { { 0.51 0.55
5 156 8 163 8 219 15 196 9 181 9 458 46 { { 0.22 0.61
0546-1725 3 141 14 201 20 324 20 391 8 692 21 1348 58 3137 80 0.97 0.88
0547-1958 2 162 8 { { 428 26 476 23 616 31 1088 109 1546 95 1.02 0.50
1 200 15 { { 428 25 465 10 661 34 943 94 1546 93 0.80 0.51
5 185 9 274 14 428 25 482 7 618 31 1014 101 1546 93 0.91 0.49
0553-1709 5 88 4 167 8 239 16 289 13 422 21 1153 44 2226 109 1.12 0.86
0559-1817 3 208 21 204 21 414 24 179 9 { { 332 17 { { -0.14 0.44
0603-1716 4 370 12 337 8 317 10 262 6 301 8 515 26 507 55 -0.33 0.28
5 523 24 452 8 317 20 338 18 227 11 380 38 507 109 -0.41 0.17
0605-1755 5 41 2 115 6 251 17 264 6 427 21 1014 101 1278 121 1.76 0.67
0606-2022 2 421 21 { { 1040 56 1268 21 1910 96 4247 425 8518 244 1.04 0.80
1 383 20 { { 1040 55 1271 23 1867 31 4344 217 8518 244 1.14 0.80
0610-1847 3 982 31 818 30 286 18 605 10 485 15 541 28 { { -0.46 -0.08
0617-1715 5 260 13 270 14 445 25 335 22 446 22 844 84 492 42 0.24 0.16
0618-2051 1 117 8 { { 267 17 324 10 466 24 713 71 1752 37 0.96 0.71
0619-2054 2 389 20 { { 590 32 624 26 846 42 1179 118 1842 92 0.45 0.46
0621-1715 3 63 9 105 16 212 15 314 8 451 14 956 50 1594 46 1.52 0.69
0623-1708 5 92 5 108 5 217 15 268 7 346 17 614 61 1080 40 1.02 0.59
0629-1959 1 1038 39 { { 784 42 769 14 699 36 724 72 592 45 -0.28 -0.11
0633-1802 3 201 21 263 26 373 22 497 10 647 20 1155 49 1642 45 0.86 0.50

36 MINGALIEV, BOTASHEV, STOLYAROV
Table 3: The uxes for the complete sample of sources (continue)
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
0636-2031 2 417 21 { { 1303 70 3040 16 4616 231 10794 1079 { { 1.88 0.90
5 509 29 976 38 1303 70 3054 24 5096 78 11037 85 { { 1.70 0.92
0636-2041 4 635 15 1043 21 1303 35 2988 13 5295 106 11607 94 6816 190 1.47 0.35
0824-1827 3 180 18 225 23 319 20 342 9 300 15 119 24 { { 0.61 -0.75
0828-1952 1 83 8 { { 212 15 247 8 323 23 997 100 2254 121 1.04 0.93
5 100 5 130 7 212 15 275 11 417 21 799 80 2254 121 0.96 0.89
0836-2017 2 3045 152 { { 1712 90 2251 31 1700 85 2431 243 10808 266 -0.29 0.66
0837-1951 1 717 11 { { 1709 89 2043 25 3273 109 { { 10972 247 0.99 0.71
0844-1846 3 160 16 191 19 245 17 248 10 299 15 351 25 { { 0.42 0.25
0847-1755 5 178 9 191 19 203 15 334 113 217 11 { { { { 0.60 -
0847-1756 5 { { { { 220 16 189 10 460 23 1048 105 2126 57 - 1.02
0847-2057 2 93 5 { { 231 16 266 12 324 16 537 54 1087 30 0.99 0.59
0852-2047 1 235 17 { { 614 34 881 15 1551 52 3511 176 7966 173 1.25 0.93
0858-1950 2 751 38 { 710 38 845 19 920 46 1386 139 3150 84 0.11 0.56
0859-1922 4 225 6 255 6 403 11 500 9 703 18 1456 73 3070 47 0.76 0.77
5 210 11 260 13 403 23 524 14 676 34 1422 142 3070 93 0.87 0.75
0902-1721 3 316 23 274 28 276 18 240 10 179 13 205 21 { { -0.26 -0.11
0904-1957 1 89 6 { { 205 15 211 7 274 20 610 61 1549 70 0.82 0.84
5 { { 180 9 205 15 221 15 266 13 545 55 1549 70 - 0.82
0906-2019 2 762 25 { { 627 34 700 16 711 36 586 59 { { -0.08 -0.13
5 { { 250 13 627 34 531 28 525 26 { { { { - -
0907-2026 5 585 22 594 25 417 24 477 11 442 22 601 60 737 31 -0.19 0.18
0909-1808 5 258 15 285 6 255 17 300 8 325 16 { { 473 34 0.14 0.19
0914-1842 3 98 15 149 15 224 16 269 11 354 18 541 28 1299 89 0.96 0.66
5 56 1 164 8 224 16 282 18 439 22 575 58 1299 89 1.54 0.65
0927-2034 1 650 23 { { 689 37 871 24 881 46 858 86 1380 65 0.28 0.19
0929-1820 3 169 17 154 15 207 15 227 9 190 13 288 29 { { 0.28 0.17
0931-1830 5 90 5 140 7 205 15 334 12 460 23 844 84 2069 152 1.24 0.77
0932-2017 2 112 6 { { 337 20 396 13 618 31 1483 148 3543 93 1.20 0.93
5 113 6 163 8 337 20 413 18 686 34 1537 154 3543 93 1.23 0.91
0935-1939 5 170 9 238 12 213 15 235 15 202 10 { { 206 50 0.31 -0.06
0939-1731 3 171 18 156 16 234 16 202 8 198 14 198 30 { { 0.16 -0.01
0945-1953 1 103 8 { { 271 18 208 7 459 24 1167 117 3056 70 0.67 1.13
0946-2020 2 167 8 { { 239 16 267 5 337 17 650 65 644 33 0.45 0.37
5 116 6 199 10 239 16 306 9 297 15 375 40 664 33 0.92 0.33
0948-1828 5 75 4 119 6 214 15 296 9 513 26 1200 120 2856 139 1.30 0.96
0953-1947 3 { { 109 16 220 16 294 9 460 14 880 38 2313 49 - 0.87
4 66 1 132 1 220 8 291 6 431 4 960 48 2313 49 1.41 0.88
5 88 4 161 8 220 16 340 10 493 25 942 91 2313 49 1.29 0.81
1006-1743 3 118 18 164 17 291 18 339 7 512 15 923 39 1971 37 1.00 0.74
5 125 6 252 13 291 18 347 9 464 23 1036 102 1971 37 0.97 0.73
1017-2016 1 165 12 { { 263 17 311 10 478 25 775 78 1645 72 0.60 0.70
1020-1924 2 99 5 { { 208 15 254 10 428 21 748 75 1908 56 0.89 0.85
5 95 5 187 9 208 15 277 13 481 24 689 69 1908 56 1.01 0.81
1023-1933 5 102 5 127 6 207 15 307 23 417 21 712 71 1411 38 1.04 0.64
1024-1838 3 580 21 621 11 760 41 770 8 768 23 949 41 1891 114 0.27 0.38
1028-2027 2 58 3 { { 229 16 311 6 456 23 1059 106 2097 64 1.59 0.81
1029-1852 5 575 15 546 21 594 33 627 12 528 26 275 28 551 35 0.08 -0.05
1035-2011 1 1150 45 { { 1024 54 767 24 755 39 1131 113 1392 65 -0.38 0.25
1036-1955 3 64 10 126 19 210 15 220 9 403 20 755 32 1600 37 1.17 0.84
5 80 4 119 6 210 15 243 8 466 23 928 93 1600 37 1.06 0.80
1040-1924 2 98 5 { { 301 19 351 8 530 27 969 97 1716 42 1.21 0.67
1048-1909 1 1138 20 { { 879 47 893 28 972 50 1530 153 2687 105 -0.23 0.47
1051-2023 2 126 6 { { 406 24 583 20 852 25 2158 216 4568 81 1.45 0.87
5 163 8 235 12 406 24 625 14 937 47 2123 148 4568 81 1.27 0.84
1052-1845 3 158 16 164 17 231 16 310 7 447 13 722 31 1996 81 0.64 0.79
5 117 6 210 11 231 16 334 10 463 23 886 89 2044 88 0.99 0.76
1105-1851 5 89 4 138 7 217 15 236 8 376 19 1124 112 1335 84 0.93 0.73
1110-1858 3 200 20 288 20 463 26 548 10 712 21 886 38 1034 203 0.96 0.27
1127-1857 3 1290 35 1094 19 1624 85 973 30 764 23 735 31 { { -0.27 -0.20
1133-1954 2 104 5 { { 290 18 350 14 683 34 1870 187 5277 154 1.15 1.15

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 37
Table 3: The uxes for the complete sample of sources (continue)
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
1 65 6 { { 290 18 382 12 674 35 1911 96 5277 154 1.67 1.11
1134-1727 5 142 7 245 12 455 26 600 20 896 45 2546 108 5910 98 1.36 0.97
1136-1733 5 271 11 344 17 491 28 581 11 704 35 1370 69 2336 43 0.72 0.59
1144-1741 3 106 16 125 19 264 17 279 3 558 17 1146 38 2964 100 0.92 1.00
1149-1943 1 97 7 { { 201 15 229 8 368 26 651 65 1514 37 0.82 0.80
1150-1930 2 123 6 { { 388 23 206 20 260 13 489 49 661 38 0.49 0.49
1151-1723 5 356 11 391 20 514 29 565 10 659 33 839 64 1109 57 0.44 0.28
1153-1816 5 103 5 130 7 227 16 240 6 401 20 621 60 406 35 0.80 0.22
1155-1804 3 97 15 123 18 240 16 290 12 521 16 1210 41 { { 1.04 1.02
1201-1852 5 57 3 80 4 246 17 217 9 346 17 604 27 656 37 1.27 0.47
1209-2032 1 731 25 { { 573 32 644 21 401 29 525 53 { { -0.12 -0.15
1211-1926 2 193 10 { { 358 21 388 13 457 23 548 55 { { 0.66 0.25
5 201 10 271 14 358 21 402 10 472 24 343 34 { { 0.66 -0.11
1215-1731 3 2892 72 2438 125 1744 91 1977 31 1603 26 1854 62 3001 48 -0.36 0.18
1240-1717 3 173 18 274 19 398 23 495 11 683 21 { { 2985 44 1.00 0.76
1243-1833 5 101 5 140 7 209 15 274 10 375 19 697 70 1690 40 0.95 0.77
1249-2055 2 { { { { 220 16 174 6 302 15 607 61 1239 50 - 0.83
1251-1717 3 197 20 192 19 259 17 186 7 163 11 573 30 { { -0.05 0.80
1254-1845 5 { { 111 6 292 18 300 21 566 28 1472 50 3275 120 - 1.01
1258-1750 5 271 22 { { 509 28 497 40 842 42 929 51 979 33 0.57 0.29
1258-1759 5 392 14 289 14 894 48 374 19 301 15 { { { { -0.05 -
1301-2020 1 80 8 { { 207 15 294 9 546 28 1563 156 3945 58 1.23 1.10
1304-1932 2 151 8 { { 319 20 348 5 459 23 918 92 1544 41 0.79 0.63
1306-1719 3 351 16 315 16 347 21 318 10 250 13 332 24 { { -0.09 0.03
1312-2027 1 121 9 { { 245 16 330 11 509 26 751 75 2094 50 0.95 0.78
5 113 6 161 8 245 16 341 12 464 23 962 96 2094 50 1.05 0.77
1315-1858 5 { { 117 6 243 16 385 27 679 34 2049 36 5996 235 - 1.16
1330-2056 2 179 9 { { 347 21 337 10 384 19 1147 115 1467 121 0.60 0.62
1 219 16 { { 347 21 388 12 460 24 1332 133 1467 121 0.54 0.56
5 233 12 245 12 347 21 361 9 386 19 798 80 1467 121 0.42 0.59
1337-1811 3 286 21 348 18 513 29 657 9 947 29 1943 65 4650 97 0.79 0.83
1342-2051 2 400 39 { { 291 18 302 7 411 21 531 53 579 30 -0.27 0.28
1 371 19 { { 291 18 306 10 415 21 596 60 579 30 -0.18 0.27
1343-1748 5 259 13 366 18 566 31 580 25 547 27 875 90 1664 114 0.76 0.44
1344-1723 5 245 12 249 12 350 21 327 10 274 14 369 37 { { 0.28 0.09
1356-1724 3 190 14 169 17 203 15 178 7 194 10 1357 58 { { -0.06 1.45
1356-1751 5 { { 176 9 287 18 387 23 651 33 2054 178 10180 463 - 1.38
1357-1744 5 815 31 1045 8 1009 54 1130 73 1185 59 { { 10180 463 0.31 0.93
1402-1840 5 252 13 305 15 201 15 438 18 483 24 690 63 { { 0.52 0.32
1413-2020 1 { { { { 232 16 326 11 531 27 1218 122 2856 49 - 0.92
1416-1705 3 174 18 185 19 305 19 239 6 233 16 { { 276 31 0.30 0.06
1419-1928 2 479 19 { { 1021 54 1096 11 1407 30 2814 281 4463 117 0.78 0.59
1421-1931 4 236 6 172 4 219 8 173 4 127 3 498 25 1195 18 -0.29 0.82
1423-1816 5 85 4 173 9 306 19 432 15 650 33 1732 205 3891 74 1.54 0.93
1425-1756 5 128 6 223 11 513 29 541 3 766 38 1871 166 2692 95 1.37 0.68
1432-1801 3 560 18 619 16 846 45 753 6 874 26 1082 46 1031 35 0.28 0.13
5 571 21 713 36 846 45 763 23 870 44 1039 66 1031 35 0.27 0.13
1454-1925 2 138 7 { { 346 21 373 17 659 33 1564 156 3538 115 0.94 0.95
1 145 11 { { 346 21 325 11 656 34 1319 132 3538 115 0.77 1.01
5 140 7 192 10 346 21 407 13 621 31 1464 46 3538 115 1.01 0.91
1455-1700 3 233 17 232 23 227 16 280 10 261 13 { { 354 29 0.17 0.10
1515-1939 2 { { { { 244 16 188 6 341 17 944 94 2130 98 - 1.02
1 57 6 { { 244 16 206 7 343 25 885 89 2130 98 1.22 0.99
5 61 3 { { 244 16 199 9 371 19 1041 49 2130 98 1.12 1.00
1525-1903 1 102 8 { { 330 20 371 12 627 32 1528 76 3028 74 1.22 0.89
1530-2013 2 { { { { 224 16 260 8 489 25 1211 121 2883 100 - 1.02
5 51 3 114 6 224 16 271 16 474 24 1315 75 2883 100 1.58 1.00
1542-1803 3 77 12 106 16 209 15 261 11 424 13 594 31 1254 40 1.16 0.66
5 93 5 147 7 209 15 281 25 341 17 516 52 1254 40 1.05 0.63
1551-1754 5 260 16 288 14 368 22 326 7 302 15 321 32 276 30 0.22 -0.07
1605-1734 3 112 17 160 16 337 20 468 9 841 25 2248 75 6011 199 1.36 1.08

38 MINGALIEV, BOTASHEV, STOLYAROV
Table 3: The uxes for the complete sample of sources (continue)
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
1607-2039 2 167 8 { { 245 17 166 8 347 17 793 79 1677 153 0.00 0.98
1 141 10 { { 245 17 230 8 383 27 1009 101 1677 153 0.46 0.84
5 180 9 158 8 245 17 210 11 295 15 692 69 1677 153 0.15 0.88
1616-1723 5 49 3 121 6 205 15 268 14 399 20 1017 26 2251 106 1.61 0.90
1619-1817 3 246 18 268 27 311 19 295 12 277 14 { { { { 0.17 -
1642-2006 1 153 11 { { 262 17 172 6 268 19 593 59 636 83 0.11 0.55
1644-1804 3 252 18 232 23 358 21 247 5 227 16 { { { { -0.02 -
5 248 12 282 14 358 21 265 19 212 11 354 35 { { 0.07 0.21
1645-1835 5 90 5 113 6 233 16 347 10 534 27 1408 115 3598 170 1.29 0.99
1647-1926 2 197 10 { { 255 17 251 15 { { 468 47 769 37 0.23 0.47
1657-2004 1 203 15 { { 215 15 253 8 290 21 { { { { 0.21 -
1658-2011 5 71 4 121 6 238 16 279 7 401 20 913 91 2477 122 1.30 0.92
1701-1903 5 375 19 326 16 301 19 313 16 279 14 456 46 944 110 -0.17 0.47
1702-1758 3 97 15 138 21 252 17 382 6 562 17 1080 46 2839 141 1.30 0.85
1703-2031 2 209 10 { { 346 21 403 7 579 29 1089 109 1940 85 0.62 0.66
1709-1728 5 642 31 760 28 570 31 755 27 583 29 297 30 529 40 0.15 -0.15
1710-2030 1 62 6 { { 210 15 288 9 386 27 958 96 2134 104 1.46 0.85
5 { { 87 4 210 15 269 8 353 18 1006 53 2134 104 - 0.87
1712-1819 3 330 24 415 21 228 16 439 7 379 19 383 39 { { 0.27 -0.10
1911-1712 3 108 16 193 19 400 23 525 13 933 28 2525 85 4393 161 1.50 0.90
1911-1908 5 117 6 159 8 238 16 267 11 299 15 277 28 948 39 0.78 0.54
1911-1921 1 184 13 { { 222 16 254 8 447 23 { { { { 0.30 -
5 { { { { 222 16 252 16 70 4 217 22 { { - -0.11
1911-2006 2 2284 26 { { 2053 99 2708 28 2695 53 3295 330 2193 117 0.16 -0.09
1917-1921 1 324 17 { { 413 24 420 13 397 28 { { 798 62 0.25 0.27
5 306 15 363 18 413 24 437 9 431 22 596 60 798 62 0.34 0.25
1925-1836 5 88 4 137 7 393 23 276 18 605 30 1863 70 4543 187 1.09 1.18
1932-1931 2 145 7 { { 380 22 453 9 746 24 1940 194 5463 235 1.08 1.05
1 92 6 { { 380 22 478 15 736 38 1860 93 5463 235 1.56 1.03
5 127 6 177 9 380 22 509 9 830 42 1972 33 5463 235 1.32 1.00
1936-1711 3 { { 75 11 200 15 130 7 250 13 761 32 { { - 1.26
1938-1749 5 223 11 237 12 274 18 256 5 197 10 { { { { 0.13 -
1948-1857 3 68 10 109 16 214 15 250 10 430 13 999 43 { { 1.23 0.99
1949-1957 1 1068 19 { { 1332 70 1331 23 1401 48 1301 130 1508 42 0.21 0.05
1952-1936 2 225 11 { { 368 22 390 16 604 30 1057 106 1743 53 0.52 0.63
5 171 9 228 11 368 22 383 14 541 27 1017 47 1743 53 0.76 0.64
1955-1925 5 71 4 95 5 350 21 286 17 632 32 1259 25 1912 106 1.32 0.80
2000-1748 5 2194 53 1970 43 2700 99 1676 44 977 49 754 75 526 47 -0.26 -0.49
2000-1921 1 319 17 { { 395 23 572 10 660 34 1056 106 1795 53 0.55 0.48
5 242 8 338 10 395 23 531 11 652 33 960 96 1795 53 0.75 0.51
2005-1822 3 543 28 482 12 529 29 509 10 575 17 985 42 1644 128 -0.06 0.49
2015-1703 5 141 7 173 9 242 16 208 11 254 13 484 48 1040 79 0.37 0.68
2022-2007 1 110 8 { { 293 18 396 22 536 28 821 82 1425 66 1.22 0.54
2022-2058 2 76 4 { { 231 16 125 6 218 11 733 73 1355 66 0.47 1.01
5 89 5 118 6 231 16 176 9 237 12 543 54 1355 66 0.64 0.86
2023-1911 5 64 3 113 6 239 16 232 12 402 20 1247 110 1754 124 1.23 0.85
2030-1702 3 51 8 79 12 225 16 252 10 445 13 1036 44 { { 1.51 1.01
2035-1745 5 42 2 102 5 214 15 253 13 439 22 996 100 2292 102 1.71 0.93
2038-2011 2 139 7 { { 374 22 277 4 524 26 1003 100 1754 88 0.66 0.78
1 155 11 { { 374 22 296 9 537 28 920 92 1754 88 0.61 0.75
5 135 7 190 10 374 22 300 6 539 27 1023 90 1754 88 0.76 0.75
2047-1821 3 111 17 160 16 266 17 325 13 505 15 1026 44 { { 1.02 0.82
2053-1838 5 51 3 89 4 201 15 220 10 430 22 573 57 2456 124 1.39 1.02
2056-1956 2 315 9 { { 1094 58 1166 4 1739 27 3610 361 7063 244 1.24 0.76
1 285 15 { { 1094 58 1148 28 1778 56 3730 186 7063 244 1.32 0.77
5 284 6 544 8 1094 58 1226 15 1851 34 3642 92 7063 244 1.39 0.74
2101-1747 3 161 16 206 21 338 20 362 11 604 18 1429 61 { { 0.77 0.98
2114-1819 5 131 7 198 10 276 18 349 15 528 26 1101 32 2070 65 0.93 0.75
2116-2055 2 271 21 { { 820 44 1106 19 1601 9 4114 411 9326 293 1.33 0.90
1 262 19 { { 820 44 1102 13 1718 25 { { 9326 293 1.36 0.90
5 259 7 431 13 820 44 1141 7 1736 33 4123 40 9326 293 1.41 0.89

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 39
Table 3: The uxes for the complete sample of sources (continue)
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
2129-1821 3 574 22 680 13 951 51 1061 14 1251 38 1520 51 1142 80 0.58 0.03
2131-2036 1 212 15 { { 608 33 791 19 1255 40 2699 135 6537 186 1.25 0.89
2135-1734 5 150 8 243 12 390 23 454 18 720 36 1376 44 2972 126 1.05 0.79
2137-2042 2 755 34 { { 1549 81 1847 21 2536 31 { { 9021 163 0.85 0.67
2138-1810 5 515 13 757 19 1056 56 1213 24 1763 42 2373 182 3161 196 0.81 0.40
2138-1843 5 222 22 307 9 504 28 677 8 931 47 2045 83 4501 99 1.06 0.80
2139-1838 3 135 14 170 17 276 18 322 4 { { 800 42 1401 91 0.82 0.62
2147-1740 5 167 8 212 11 372 22 464 12 768 38 1453 30 3199 117 0.97 0.82
2148-1723 5 1119 11 1208 10 697 38 1292 16 1029 51 695 37 1583 77 0.14 0.09
2149-1859 4 { { 61 2 245 9 184 5 335 8 { { 990 66 - 0.71
5 { { 77 4 245 17 166 8 289 14 760 80 990 132 - 0.75
2149-1912 1 107 8 { { 202 15 249 8 424 22 { { 1603 95 0.80 0.79
2151-1946 2 339 12 { { 767 41 940 8 1335 29 2759 276 5067 104 0.97 0.71
2156-1813 3 121 18 { { 564 31 523 9 915 28 2334 78 5322 312 1.39 0.98
5 { { { { 564 31 436 22 906 54 2206 52 5322 312 - 1.06
2157-1807 5 281 5 435 10 554 31 743 22 1128 55 1834 36 1994 69 0.92 0.42
2206-1800 5 91 5 150 8 201 15 212 5 421 21 510 51 1288 118 0.80 0.76
2206-1835 4 3116 87 3636 83 4271 50 4750 41 5600 140 7239 362 10019 95 0.40 0.32
5 2882 59 3617 35 4271 99 5130 50 5340 94 7208 73 10019 189 0.55 0.28
2214-1701 3 586 23 1059 12 2668 99 3008 28 5385 27 13077 229 18407 639 1.55 0.76
2233-2024 2 90 5 { { 225 16 252 9 300 15 517 52 898 32 0.98 0.54
2234-2055 4 378 18 383 10 317 10 366 11 279 7 365 18 454 39 -0.03 0.09
2235-1826 5 129 7 142 7 215 15 181 9 115 6 { { 251 40 0.32 0.14
2236-1706 3 341 19 319 16 332 20 326 10 332 17 414 62 { { -0.04 0.17
2237-1712 5 113 6 178 9 347 21 501 10 832 42 2150 46 4759 99 1.41 0.95
2239-1720 5 62 3 126 6 644 35 432 6 926 46 2351 76 1977 94 1.84 0.64
2245-1737 5 121 6 179 9 217 15 229 11 354 18 281 28 940 77 0.61 0.60
2251-1848 3 139 14 169 17 231 16 276 8 346 17 467 47 967 51 0.65 0.53
4 132 3 188 5 231 8 277 4 334 8 490 25 967 51 0.70 0.53
2252-2047 1 141 10 { { 236 16 228 8 265 19 { { { { 0.45 -
5 145 7 174 9 236 16 265 13 227 11 132 13 { { 0.57 -0.50
2256-2011 2 552 8 { { 454 26 507 10 419 21 314 31 { { -0.08 -0.34
2257-1828 5 { { { { 267 17 189 9 400 20 585 59 1644 137 - 0.91
2303-1841 3 579 19 457 12 766 41 661 12 863 26 1757 75 864 78 0.13 0.11
2304-1939 1 102 8 { { 217 15 232 8 296 21 454 45 975 91 0.78 0.61
5 118 6 123 6 217 15 257 29 293 15 514 51 975 91 0.74 0.56
2315-1800 5 338 6 463 14 665 36 747 9 947 47 1563 38 2735 89 0.75 0.55
2320-1919 1 166 12 { { 382 22 475 18 566 29 1117 112 3188 123 1.00 0.80
5 226 11 269 14 382 22 505 20 616 31 1159 28 3188 123 0.76 0.78
2329-1923 2 132 7 { { 483 27 526 8 836 11 1983 198 4275 122 1.31 0.88
2330-1808 3 95 14 117 18 202 15 250 10 369 18 724 73 2201 102 0.92 0.92
5 83 4 143 7 202 15 250 12 434 22 853 38 2201 102 1.05 0.92
2337-1752 5 331 10 465 26 618 34 696 8 872 44 1309 46 2314 49 0.70 0.51
2347-1856 3 297 16 357 18 523 29 596 9 709 21 489 74 { { 0.66 -0.14
5 286 12 425 12 523 29 648 16 680 34 600 60 { { 0.77 -0.05
2355-1810 5 88 4 153 8 305 19 391 20 571 29 1387 52 1641 128 1.41 0.61
2357-1817 5 56 3 144 7 240 16 308 14 536 27 1126 79 2644 124 1.62 0.91
2359-2048 2 167 8 { { 256 17 277 13 368 18 681 68 1023 52 0.48 0.55

40 MINGALIEV, BOTASHEV, STOLYAROV
100
1000
0001­1741 Dec95
Flux
density,
mJy
1000
0003­1727 Oct96
100
0003­1941 Jul95
100
1000
0009­2056 Aug95
0009­2056 Oct96
100
0015­1807 Oct96
100
Flux
density,
mJy
0015­1812 Dec95
0015­1812 Oct96
100
1000
0015­1929 Jul95
100
1000
0020­2014 Oct96
1 10
100
1000
Frequency, GHz
Flux
density,
mJy
0021­1910 Aug95
0021­1910 Oct96
1 10
100
1000
Frequency, GHz
0026­2004 Jul95
1 10
100
1000
Frequency, GHz
0034­1759 Dec95
100
1000
Flux
density,
mJy
0008­1939 Oct96
Figure 4: The spectra of the complete sample of sources from PMN survey.

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 41
100
1000
10000
0035­2004 Jul95
0035­2004 Oct96
Flux
density,
mJy
100
0039­1854 Oct96
100
1000
0040­2043 Aug95
0040­2043 Oct96
100
Flux
density,
mJy
0054­1952 Jul95
0054­1952 Aug95
0054­1952 Oct96
100
1000
0059­1700 Dec95
100
1000
0100­1749 Oct96
1000
10000
Flux
density,
mJy
0116­2052 Jul95
0116­2052 Oct96
1000
0118­1849 Dec95
100
1000
0119­1940 Aug95
0119­1940 Oct96
1 10
1000
Frequency, GHz
Flux
density,
mJy
0135­2008 Jul95
0135­2008 Aug95
0135­2008 Oct96
1 10
100
1000
Frequency, GHz
0140­1729 Oct96
1 10
100
Frequency, GHz
0142­1714 Dec95
Figure 4: | continued

42 MINGALIEV, BOTASHEV, STOLYAROV
100
0151­1732 Oct96
Flux
density,
mJy
100
0202­1948 Aug95
0202­1948 Jul95
0202­1948 Oct96
1000
0204­1701 Dec95
100
1000
Flux
density,
mJy
0205­1801 Oct96
100
1000
0219­1842 Dec95
0219­1842 Oct96
100
1000
0227­1713 Oct96
100
1000
Flux
density,
mJy
0231­2040 Jul95
0231­2040 Oct96
100
1000
0248­2002 Jul95
0248­2002 Oct96
100
1000
0249­1928 Dec95
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
0255­2027 Oct96
1 10
100
1000
Frequency, GHz
0307­1748 Dec95
0307­1748 Oct96
1 10
100
1000
Frequency, GHz
0320­1702 Oct96
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 43
100
1000
Flux
density,
mJy
0325­1802 Dec95
0325­1802 Oct96
100
1000
0335­1832 Oct96
100
1000
0354­1755 Oct96
100
1000
Flux
density,
mJy
0405­1831 Jan96
0405­1831 Oct96
100
0406­1749 Oct96
1000
0409­1757 Dec95
100
1000
Flux
density,
mJy
0415­2022 Jul95
1000
0416­1851 Oct96
1000
0416­2056 Aug95
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
0425­1700 Dec95
0425­1700 Oct96
1 10
100
1000
Frequency, GHz
0431­1704 Oct96
1 10
1000
Frequency, GHz
0437­1844 Dec95
Figure 4: | continued

44 MINGALIEV, BOTASHEV, STOLYAROV
100
1000
Flux
density,
mJy
0438­2012 Jul95
0438­2012 Oct96
100
1000
0444­1822 Oct96
100
1000
0444­2051 Aug95
100
1000
Flux
density,
mJy
0448­2032 Jul95
100
0450­1837 Dec95
100
1000
0451­1730 Oct96
1000
10000
Flux
density,
mJy
0455­2034 Jul95
100
1000
0501­1706 Dec95
0501­1706 Oct96
100
1000
0514­1957 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
0514­2029 Jul95
1 10
100
Frequency, GHz
0517­1756 Dec95
1 10
100
Frequency, GHz
0521­1737 Oct96
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 45
100
1000
10000
Flux
density,
mJy
0521­2047 Aug95
0521­2047 Oct96
100
0525­2010 Jul95
0525­2010 Oct96
100
1000
0546­1725 Dec95
100
1000
Flux
density,
mJy
0547­1958 Aug95
0547­1958 Jul95
0547­1958 Oct96
100
1000
0553­1709 Oct96
100
0559­1817 Dec95
100
1000
Flux
density,
mJy
0603­1716 Jan96
0603­1716 Oct96
100
1000
0605­1755 Oct96
1000
10000
0606­2022 Aug95
0606­2022 Jul95
1 10
1000
Flux
density,
mJy
Frequency, GHz
0610­1847 Dec95
1 10
100
1000
Frequency, GHz
0617­1715 Oct96
1 10
100
1000
Frequency, GHz
0618­2051 Jul95
Figure 4: | continued

46 MINGALIEV, BOTASHEV, STOLYAROV
1000
Flux
density,
mJy
0619­2054 Aug95
100
1000
0621­1715 Dec95
100
1000
0623­1708 Oct96
1000
Flux
density,
mJy
0629­1959 Jul95
100
1000
0633­1802 Dec95
1000
10000
0636­2031 Aug95
0636­2031 Oct96
1000
10000
Flux
density,
mJy
0636­2041 Jan96
100
0824­1827 Dec95
100
1000
0828­1952 Jul95
0828­1952 Oct96
1 10
1000
10000
Flux
density,
mJy
Frequency, GHz
0836­2017 Aug95
1 10
1000
10000
Frequency, GHz
0837­1951 Jul95
1 10
100
Frequency, GHz
0844­1846 Dec95
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 47
100
Flux
density,
mJy
0847­1755 Oct96
100
1000
0847­1756 Oct96
100
1000
0847­2057 Aug95
100
1000
10000
Flux
density,
mJy
0852­2047 Jul95
1000
0858­1950 Aug95
100
1000
0859­1922 Jan96
0859­1922 Oct96
100
Flux
density,
mJy
0902­1721 Dec95
100
1000
0904­1957 Jul95
0904­1957 Oct96
1000
0906­2019 Aug95
0906­2019 Oct96
1 10
1000
Flux
density,
mJy
Frequency, GHz
0907­2026 Oct96
1 10
100
1000
Frequency, GHz
0909­1808 Oct96
1 10
100
1000
Frequency, GHz
0914­1842 Dec95
0914­1842 Oct96
Figure 4: | continued

48 MINGALIEV, BOTASHEV, STOLYAROV
1000
Flux
density,
mJy
0927­2034 Jul95
100
0929­1820 Dec95
100
1000
0931­1830 Oct96
100
1000
Flux
density,
mJy
0932­2017 Aug95
0932­2017 Oct96
100
0935­1939 Oct96
100
0939­1731 Dec95
100
1000
Flux
density,
mJy
0945­1953 Jul95
100
1000
0946­2020 Aug95
0946­2020 Oct96
100
1000
0948­1828 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
0953­1947 Dec95
0953­1947 Jan96
0953­1947 Oct96
1 10
100
1000
Frequency, GHz
1006­1743 Dec95
1006­1743 Oct96
1 10
100
1000
Frequency, GHz
1017­2016 Jul95
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 49
100
1000
Flux
density,
mJy
1020­1924 Oct96
100
1000
1023­1933 Oct96
100
1000
1024­1838 Dec95
100
1000
Flux
density,
mJy
1028­2027 Aug95
100
1000
1029­1852 Oct96
100
1000
1035­2011 Jul95
100
1000
Flux
density,
mJy
1036­1955 Dec95
1036­1955 Oct96
100
1000
1040­1924 Aug95
100
1000
1048­1909 Jul95
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
1051­2023 Aug95
1051­2023 Oct96
1 10
100
1000
Frequency, GHz
1052­1845 Dec95
1052­1845 Oct96
1 10
100
1000
Frequency, GHz
1105­1851 Oct96
Figure 4: | continued

50 MINGALIEV, BOTASHEV, STOLYAROV
100
1000
Flux
density,
mJy
1110­1858 Dec95
1000
1127­1857 Dec95
100
1000
1133­1954 Aug95
1133­1954 Jul95
100
1000
Flux
density,
mJy
1134­1727 Oct96
100
1000
1136­1733 Oct96
100
1000
1144­1741 Dec95
100
1000
Flux
density,
mJy
1149­1943 Jul95
100
1000
1150­1930 Aug95
1000
1151­1723 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
1153­1816 Oct96
1 10
100
1000
Frequency, GHz
1155­1804 Dec95
1 10
100
1000
Frequency, GHz
1201­1852 Oct96
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 51
100
1000
Flux
density,
mJy
1209­2032 Jul95
100
1000
1211­1926 Aug95
1211­1926 Oct96
1000
1215­1731 Dec95
100
1000
Flux
density,
mJy
1240­1717 Dec95
100
1000
1243­1833 Oct96
100
1000
1249­2055 Aug95
100
1000
Flux
density,
mJy
1251­1717 Dec95
100
1000
1254­1845 Oct96
100
1000
1258­1750 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
1258­1759 Oct96
1 10
100
1000
Frequency, GHz
1301­2020 Jul95
1 10
100
1000
Frequency, GHz
1304­1932 Aug95
Figure 4: | continued

52 MINGALIEV, BOTASHEV, STOLYAROV
100
1000
Flux
density,
mJy
1306­1719 Dec95
100
1000
1312­2027 Jul95
1312­2027 Oct96
100
1000
10000
1315­1858 Oct96
100
1000
Flux
density,
mJy
1330­2056 Aug95
1330­2056 Jul95
1330­2056 Oct96
100
1000
1337­1811 Dec95
100
1000
1342­2051 Aug95
1342­2051 Jul95
100
1000
Flux
density,
mJy
1343­1748 Oct96
100
1000
1344­1723 Oct96
100
1000
0354­1755 Dec95
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
1356­1724 Dec95
1 10
100
1000
10000
Frequency, GHz
1356­1751 Oct96
1 10
1000
10000
Frequency, GHz
1357­1744 Oct96
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 53
100
1000
Flux
density,
mJy
1402­1840 Oct96
100
1000
1413­2020 Jul95
100
1000
1416­1705 Dec95
1000
Flux
density,
mJy
1419­1928 Aug95
100
1000
1421­1931 Jan96
100
1000
1423­1816 Oct96
100
1000
Flux
density,
mJy
1425­1756 Oct96
1000
1432­1801 Dec95
1432­1801 Oct96
100
1000
1454­1925 Aug95
1454­1925 Jul95
1454­1925 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
1455­1700 Dec95
1 10
100
1000
Frequency, GHz
1515­1939 Aug95
1515­1939 Jul95
1515­1939 Oct96
1 10
100
1000
Frequency, GHz
1525­1903 Jul95
Figure 4: | continued

54 MINGALIEV, BOTASHEV, STOLYAROV
100
1000
Flux
density,
mJy
1530­2013 Aug95
1530­2013 Oct96
100
1000
1542­1803 Dec95
1542­1803 Oct96
100
1551­1754 Oct96
100
1000
10000
Flux
density,
mJy
1605­1734 Dec95
100
1000
1607­2039 Aug95
1607­2039 Jul95
1607­2039 Oct96
100
1000
1616­1723 Oct96
100
Flux
density,
mJy
1619­1817 Dec95
100
1000
1642­2006 Jul95
100
1644­1804 Dec95
1644­1804 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
1645­1835 Oct96
1 10
100
1000
Frequency, GHz
1647­1926 Aug95
1 10
100
Frequency, GHz
1657­2004 Jul95
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 55
100
1000
Flux
density,
mJy
1658­2011 Oct96
100
1000
1701­1903 Oct96
100
1000
1702­1758 Dec95
100
1000
Flux
density,
mJy
1703­2031 Aug95
100
1000
1709­1728 Oct96
100
1000
1710­2030 Jul95
1710­2030 Oct96
100
Flux
density,
mJy
1712­1819 Dec95
100
1000
1911­1712 Dec95
100
1000
1911­1908 Oct96
1 10
100
Flux
density,
mJy
Frequency, GHz
1911­1921 Jul95
1911­1921 Oct96
1 10
1000
Frequency, GHz
1911­2006 Aug95
1 10
1000
Frequency, GHz
1917­1921 Jul95
1917­1921 Oct96
Figure 4: | continued

56 MINGALIEV, BOTASHEV, STOLYAROV
100
1000
10000
Flux
density,
mJy
1925­1836 Oct96
100
1000
10000
1932­1931 Aug95
1932­1931 Jul95
1932­1931 Oct96
100
1000
1936­1711 Dec95
100
Flux
density,
mJy
1938­1749 Oct96
100
1000
1948­1857 Dec95
1000
1949­1957 Jul95
100
1000
Flux
density,
mJy
1952­1936 Aug95
1952­1936 Oct96
100
1000
1955­1925 Oct96
1000
2000­1748 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
2000­1921 Jul95
2000­1921 Oct96
1 10
1000
Frequency, GHz
2005­1822 Dec95
1 10
100
1000
Frequency, GHz
2015­1703 Oct96
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 57
100
1000
Flux
density,
mJy
2022­2007 Jul95
100
1000
2022­2058 Aug95
2022­2058 Oct96
100
1000
2023­1911 Oct96
100
1000
Flux
density,
mJy
2030­1702 Dec95
100
1000
2035­1745 Oct96
100
1000
2038­2011 Aug95
2038­2011 Jul95
2038­2011 Oct96
100
1000
Flux
density,
mJy
2047­1821 Dec95
100
1000
2053­1838 Oct96
1000
10000
2056­1956 Aug95
2056­1956 Jul95
2056­1956 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
2101­1747 Dec95
1 10
100
1000
Frequency, GHz
2114­1819 Oct96
1 10
100
1000
10000
Frequency, GHz
2116­2055 Aug95
2116­2055 Jul95
2116­2055 Oct96
Figure 4: | continued

58 MINGALIEV, BOTASHEV, STOLYAROV
1000
Flux
density,
mJy
2129­1821 Dec95
100
1000
10000
2131­2036 Jul95
100
1000
2135­1734 Oct96
1000
10000
Flux
density,
mJy
2137­2042 Aug95
1000
2138­1810 Oct96
100
1000
2138­1843 Oct96
100
1000
Flux
density,
mJy
2139­1838 Dec95
100
1000
2147­1740 Oct96
1000
2148­1723 Oct96
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
2149­1859 Jan96
2149­1859 Oct96
1 10
100
1000
Frequency, GHz
2149­1912 Jul95
1 10
1000
Frequency, GHz
2151­1946 Aug95
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 59
100
1000
10000
Flux
density,
mJy
2156­1813 Dec95
2156­1813 Oct96
1000
2157­1807 Oct96
100
1000
2206­1800 Oct96
10000
Flux
density,
mJy
2206­1835 Jan96
2206­1835 Oct96
1000
10000
2214­1701 Dec95
100
1000
2233­2024 Aug95
100
1000
Flux
density,
mJy
2234­2055 Jan96
100
2235­1826 Oct96
100
1000
2236­1706 Dec95
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
2237­1712 Oct96
1 10
100
1000
Frequency, GHz
2239­1720 Oct96
1 10
100
1000
Frequency, GHz
2245­1737 Oct96
Figure 4: | continued

60 MINGALIEV, BOTASHEV, STOLYAROV
100
1000
Flux
density,
mJy
2251­1848 Dec95
2251­1848 Jan96
100
2252­2047 Jul95
2252­2047 Oct96
1000 2256­2011 Aug95
100
1000
Flux
density,
mJy
2257­1828 Oct96
1000
2303­1841 Dec95
100
1000
2304­1939 Jul95
2304­1939 Oct96
1000
Flux
density,
mJy
2315­1800 Oct96
100
1000
2320­1919 Jul95
2320­1919 Oct96
100
1000
2329­1923 Aug95
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
2330­1808 Dec95
2330­1808 Oct96
1 10
1000
Frequency, GHz
2337­1752 Oct96
1 10
1000
Frequency, GHz
2347­1856 Dec95
2347­1856 Oct96
Figure 4: | continued

SIMULTANEOUS SPECTRA OF COMPLETE SAMPLE OF SOURCES 61
1 10
100
1000
Flux
density,
mJy
Frequency, GHz
2355­1810 Oct96
1 10
100
1000
&RPPHQWV#WR#WKH#)LJ###
##-XO\#####
##$XJXVW#####
##'HFHPEHU#####
##-DQXDU\#####
##2FWREHU#####
##)OX[HV#IURP#7(;$6########*+]##DQG#301#######*+]##VXUYH\V
Frequency, GHz
2357­1817 Oct96
1 10
100
1000
Frequency, GHz
2359­2048 Aug95
Figure 4: | continued