Table 1: Overall properties of the sample galaxies$^\star $.
      Radio properties Optical properties
IAU name1 RA2 Dec2 Morphology3 $\alpha$ Flux4 Magnitude z Observations5
  [J 2000] [J 2000] (Size)   [Jy]      
0001+058 (oo) 00 04 01.48 +06 07 31.0 D ($\sim$ $7\hbox{$^{\prime\prime}$ }$) -1.16 1.28 $R\sim 24$ ... I3, c
0018+052 (oo) 00 20 56.29 +05 33 25.4 T ( $12\hbox{$^{\prime\prime}$ }$) -1.38 1.78 R>23.0 ... I2, c
0030+061 (mg) 00 33 15.28 +06 28 18.0 R ( $3\hbox{$^{\prime\prime}$ }$) -1.20 3.09 R>23.0 ... I2, b
0048+072 (oo) 00 51 28.03 +07 28 55.4 D ( $20\hbox{$^{\prime\prime}$ }$) -1.12 1.96 $R=21.9\pm 0.1$ ... I3, a
0127-195 (ml) 01 30 00.38 -19 17 11.1 SR ($\sim$ $1\hbox{$^{\prime\prime}$ }$) -1.41 0.30 R>23.0 ... I2, b
0321-042 (gb) 03 24 21.03 -04 05 03.8 SR ($\sim$ $1\hbox{$^{\prime\prime}$ }$) -1.20 0.87 $B=22.4\pm 0.1$ 2.53 I1, S3, S4, S6, a
0348+013 (gb) 03 50 57.37 +01 31 04.6 D ($\sim$ $8\hbox{$^{\prime\prime}$ }$) -1.20 1.02 $R=18.9\pm 0.1$ 1.12 I1, S1, S2, S3, a
0355-037 (gb) 03 57 47.91 -03 34 07.9 D ( $12\hbox{$^{\prime\prime}$ }$) -1.27 1.05 $R=23.3\pm 0.3$ ... I1, a
0410-198 (ml) 04 12 29.21 -19 42 08.8 D ( $11\hbox{$^{\prime\prime}$ }$) -1.18 2.23 $R=20.9\pm 0.2$ 0.79 published
0423-199 (ml) 04 25 44.33 -19 50 25.2 D ( $3\hbox{$^{\prime\prime}$ }$) -1.25 0.92 $R=23.1\pm 0.2$ 1.12 I2, S3, S6, a
0424-197 (ml) 04 26 37.62 -19 37 48.2 SR ($\sim$ $1\hbox{$^{\prime\prime}$ }$) -1.20 0.38 $R=22.0\pm 0.3$ ... I2, a, $\ast$
0430-197 (ml) 04 32 28.30 -19 40 45.2 R ( $2\hbox{$^{\prime\prime}$ }$) -1.20 0.47 R>22.7 ... I2, a
0441+049 (gb) 04 44 17.94 +05 01 25.6 D ( $12\hbox{$^{\prime\prime}$ }$) -1.10 0.83 $R\sim 23$ ... I1, b
0449-195 (ml) 04 51 13.15 -19 29 11.3 SR ($\sim$ $1\hbox{$^{\prime\prime}$ }$) -1.22 0.24 R>23.3 ... I1, a
0551-196 (ml) 05 53 11.06 -19 36 53.4 D? ( $34\hbox{$^{\prime\prime}$ }$) -1.31 0.48 $R=22.3\pm 0.2$ ... I2, a, $\ast$
0634-196 (ml) 06 36 28.68 -19 38 47.2 SR ($\sim$ $1\hbox{$^{\prime\prime}$ }$) -1.24 0.60 R>24 ... I2, a
0852+124 (oo) 08 55 21.37 +12 17 26.3 D ( $15\hbox{$^{\prime\prime}$ }$) -1.28 1.05 $V=23.3\pm 0.4$ 2.47 published
0918-194 (ml) 09 21 15.49 -19 37 37.4 D ( $29\hbox{$^{\prime\prime}$ }$) -1.20 0.30 $R=22.7\pm 0.3$ ... I2, a
0946+077 (mg) 09 48 55.25 +07 28 09.2 R ( $5\hbox{$^{\prime\prime}$ }$) -1.14 1.99 R>23.3 ... I2, a
1005-046 (gb) 10 07 49.30 -04 53 42.0 T ( $100\hbox{$^{\prime\prime}$ }$) -1.13 1.08 $R=20.2\pm 0.1$ 0.62 I4, S1, a
1048+002 (gb) 10 50 40.35 -00 03 53.9 D ( $7\hbox{$^{\prime\prime}$ }$) -1.22 3.46 $R=22.3\pm 0.2$ 0.71 I2, S1, S4, a
1059+107 (gb) 11 02 17.42 +10 29 07.5 T ( $6\hbox{$^{\prime\prime}$ }$) -1.42 3.50 $R=21.9\pm 0.1$ ... I4, b
1132+112 (ml) 11 35 21.10 +10 56 19.3 D ( $8\hbox{$^{\prime\prime}$ }$) -1.26 0.97 $R=22.0\pm 0.1$ ... I6, a
1146+052 (mg) 11 48 47.78 +04 55 25.2 D ( $41\hbox{$^{\prime\prime}$ }$) -1.13 2.65 $R=22.6\pm 0.1$ 0.42 I4, S1, S3, S5, b
1224-085 (oo) 12 27 03.73 -08 48 26.7 D ( $7\hbox{$^{\prime\prime}$ }$) -1.20 1.23 $R\sim 22$ ... I4, c, $\ast$
1238-074 (oo) 12 40 47.82 -07 43 13.9 SR ($\sim$ $2\hbox{$^{\prime\prime}$ }$) -1.12 (0.6) $R=23.3\pm 0.3$ ... I6, a
1245+115 (ml) 12 48 17.16 +11 17 22.9 SR ($\sim$ $2\hbox{$^{\prime\prime}$ }$) -1.48 1.15 $R=21.3\pm 0.1$ ... I6, b
1246-081 (oo) 12 48 51.32 -08 22 27.7 SR ($\sim$ $1\hbox{$^{\prime\prime}$ }$) -1.37 (1.0) $R=22.8\pm 0.4$ ... I2, a
1248-108 (oo) 12 50 40.00 -11 05 34.1 T ( $10\hbox{$^{\prime\prime}$ }$) -1.36 (0.8) $R=22.7\pm 0.3$ ... I2, a
1317-194 (ml) 13 20 11.83 -19 42 29.0 T ( $24\hbox{$^{\prime\prime}$ }$) -1.22 0.23 $R=24.4\pm 0.2$ ... I4, a
1324-104 (oo) 13 26 47.77 -10 40 50.6 D ( $6\hbox{$^{\prime\prime}$ }$) -1.28 (0.55) $R=22.3\pm 0.2$ ... I2, b
1329-195 (ml) 13 31 47.13 -19 47 26.3 SR ($\sim$ $2\hbox{$^{\prime\prime}$ }$) -1.28 0.35 $R=22.3\pm 0.2$ 0.98 I2, S1, b
1411-192 (oo) 14 14 22.97 -19 27 54.8 D ($\sim$ $12\hbox{$^{\prime\prime}$ }$) -1.27 1.33 $R\sim 22.6$ 0.48 published
1443-198 (ml) 14 46 48.31 -20 03 38.0 D/T ( $7\hbox{$^{\prime\prime}$ }$) -1.27 0.95 $R\sim 20.9$ 0.75 published
1509-158 (oo) 15 12 31.02 -16 00 04.1 U (< $5\hbox{$^{\prime\prime}$ }$) -1.24 1.03 R>24 ... I2, b
1523-017 (mg) 15 26 30.99 -01 54 13.8 T ( $12\hbox{$^{\prime\prime}$ }$) -1.04 2.07 $R=21.9\pm 0.2$ 0.93 I2, S1, S3, b
1612-208 (oo) 16 15 56.00 -20 58 09.3 U (< $5\hbox{$^{\prime\prime}$ }$) -1.22 (0.35) $R=22.0\pm 0.2$ ... I2, a, $\ast$
1621-196 (oo) 16 24 35.55 -19 47 15.6 T ( $19\hbox{$^{\prime\prime}$ }$) -1.37 (0.55) $R=21.6\pm 0.2$ ... I2, a, $\ast$
1623-194 (oo) 16 26 24.90 -19 35 04.8 D ( $11\hbox{$^{\prime\prime}$ }$) -1.12 0.98 $R=22.5\pm 0.2$ ... I2, a, $\ast$
1631-222 (oo) 16 34 49.82 -22 22 11.5 U (< $5\hbox{$^{\prime\prime}$ }$) -1.46 4.28 $R=25.5\pm 0.4$ ... I2, b
1632-199 (oo) 16 35 45.45 -20 04 18.0 SR ($\sim$ $3\hbox{$^{\prime\prime}$ }$) -1.05 0.96 R>23.4 ... I2, b
1859-187 (oo) 19 02 05.59 -18 43 31.6 D ( $26\hbox{$^{\prime\prime}$ }$) -1.39 (0.65) $R=22.9\pm 0.2$ ... I2, b
2011-169 (oo) 20 14 38.28 -16 48 21.7 SR ($\sim$ $1\hbox{$^{\prime\prime}$ }$) -1.05 (0.60) R>25.6 ... I2, a
2023-156 (oo) 20 26 42.31 -15 30 04.3 D ( $9\hbox{$^{\prime\prime}$ }$) -1.44 (0.9) $R=23.6\pm 0.3$ ... I2, b, $\ast$
2057-179 (oo) 21 00 15.18 -17 45 50.7 D ( $10\hbox{$^{\prime\prime}$ }$) -1.15 3.04 $R=21.5\pm 0.3$ 0.92 I5, S7, a
2105-119 (oo) 21 08 18.83 -11 41 56.2 D ($\sim$ $4\hbox{$^{\prime\prime}$ }$) -1.20 0.87 $R=24.3\pm 0.3$ ... I2, b
2222-057 (oo) 22 25 03.91 -05 29 56.0 D ( $8\hbox{$^{\prime\prime}$ }$) -1.16 (0.55) R>23 ... I5, a
2232-062 (oo) 22 35 07.87 -05 58 37.5 D ( $11\hbox{$^{\prime\prime}$ }$) -1.10 (0.8) $R\sim 23.5$ ... I3, b
2236-039 (oo) 22 39 03.60 -03 38 57.9 R ( $3\hbox{$^{\prime\prime}$ }$) -1.26 0.99 $R\sim 23$ ... I3, b, $\ast$
2236-047 (oo) 22 39 32.73 -04 29 32.0 D ( $15\hbox{$^{\prime\prime}$ }$) -1.42 2.94 $R\sim 22.3$ 0.55 published
2245-037 (oo) 22 47 37.16 -03 31 37.7 see text -1.05 (0.35) see text ... I3, a
2347+015 (oo) 23 49 42.00 +01 50 55.2 R ($\sim$ $4\hbox{$^{\prime\prime}$ }$) -1.16 (0.30) $R=22.8\pm 0.4$ ... I2, a, $\ast$
Notes:
$^\star $ Detailed information about each source is given in Sect. 3.
1 The characters in parenthesis after the IAU names codify the radio survey from where the object was selected as follows:
(oo) Ooty lunar occultation survey at 327 MHz; (ml) Molonglo surveys (MC 1 and MC 2) at 408 MHz; (mg) MIT (365 MHz) - Green-Bank (4.8 GHz) survey; (gb) Green-Bank (1.4 GHz) - Molonglo (408 MHz) survey.
2 The positions refer to the radio peak for unresolved sources and to the central radio component if detected. For the remaining sources, the mid-point between the lobes is adopted (see Fig. 1).
3 Radio morphology: D (Double), T (Triple), SR (Slightly Resolved), R (Resolved), U (Unresolved).
4 The radio fluxes are given at 408 MHz, except the values in parenthesis that correspond to 327 MHz.
5 The codes for the optical observations (I, S) are as defined in Tables 2 and 3. Exposure times for imaging ranged between ten and 30 min at the ESO 3.6 m/NTT 3.5 m telescopes, and 20 and 60 min at the ESO 2.2 m/Danish 1.5 m telescopes. Exposure times for spectroscopy are given together with the comments for each source. The letters "a'', "b'' and "c'' refer to the quality of the astrometry as described in Sect. 2.3. Asterisks refer to the sources for which our spectroscopic data did not yield redshift (see Sect. 2.5). References to published observations are given in Sect. 3.

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations
3 Comments on individual systems
4 Conclusions
References
Online Material
List of tables
List of figures