Table 1: The sample of radio-loud quasars.
No. Object Name Type z MR(host) MR(QSO) Reference $L_{\rm 5~ GHz}^{\rm ext}$   Reference
(1)    (2)   (3) (4) (5)         (6)         (7) (8) (9)      (10)
1 0133+207" 3C 47 S 0.425 -23.57 -24.27 2 26.71 6
2 0137+012" PHL 1093 S 0.258 -23.74 -23.67 2 27.07 7
3 0137+3309 3C 48 S 0.367 -25.03 -25.92 2 27.52 6
4 0202-765" PKS S 0.389 -23.32 -25.18 2 ...  
5 0312-770" PKS F 0.223 -23.98 -24.60 2 ...  
6 0340+048" 3C 93 S 0.357 -23.93 -23.71 2 25.56 8
7 0405-123" OF-109 F 0.573 -23.97 -27.87 1 27.16 6
8 0454-22"" PKS S 0.533 -21.39 -26.79 1 27.57 9
9 0736+01"" OI+061 F 0.191 -23.78 -24.23 2 24.32 6
10 0837-120" 3C 206 S 0.198 -23.29 -24.23 2 26.03 6
11 0903+169" 3C 215 S 0.412 -23.28 -24.28 2 26.51 6
12 1004+130" 4C 13.41 S 0.240 -24.26 -25.82 2 26.15 6
13 1020-103" OL-133 S 0.197 -23.36 -23.47 3 24.83 13
14 1138+0003 LBQS ? 0.500 -23.97 -24.35 4 ...  
15 1217+023" ON+029 F 0.239 -23.71 -24.40 3 25.45 6
16 1218+1734 LBQS   Sa 0.445 -23.46 -23.74 2 25.93 14
17 1222+1235 LBQS   Sb 0.412 -24.02 -24.24 2 25.96 14
18 1226+023" 3C 273 F 0.158 -24.44 -27.39 2 27.04 6
19 1230-0015 LBQS S 0.470 -23.14 -24.64 4 ...  
20 1250+568" 3C 277.1 S 0.321 -22.96 -23.29 2 26.73 6
21 1302-102" OP-106 S 0.286 -24.34 -26.13 2 25.70 6
22 1309+355" Ton 1565 F 0.184 -23.82 -24.73 2 24.14 6
23 1425+267" Ton 202 S 0.366 -23.65 -25.69 2 25.78 6
24 1512+37"" 4C 37.43 S 0.371 -23.86 -25.58 2 26.28 6
25 1545+210" 3C 323.1 S 0.266 -23.53 -25.14 2 26.42 6
26 1548+114A 4C+11.50 F 0.436 -22.40 -23.86 2 25.06 10
27 1641+399" 3C 345 F 0.593 -23.75 -26.35 1 26.48 11
28 1704+608" 3C 351 S 0.371 -24.79 -26.16 2 26.76 6
29 2128-123" OX-148 F 0.501 -22.82 -27.11 5 ...  
30 2135-147" PHL 1657 S 0.200 -23.43 -24.16 2 26.34 6
31 2141+175" OX 169 F 0.213 -23.38 -24.79 2 26.33 6
32 2201+315" 4C 31.63 F 0.295 -24.70 -25.98 2 26.54 6
33 2247+140" 4C 14.82 S 0.237 -23.52 -24.10 2 ...  
34 2348+0210 LBQS ? 0.504 -23.75 -25.13 4 ...  
35 2349-014" PB 5564 S 0.173 -24.27 -24.02 2 ...  
36 2351-0036 LBQS F 0.460 -23.02 -24.18 4 ...  
37 2355-082" PHL 6113 S 0.210 -23.62 -23.06 3 28.01 12
NOTES - Column (1) number; Col. (2): object; Col. (3): common name; Col. (4): type (based on the spectral index between 1.4 and 5 GHz; Col. (5): redshift; Col. (6) R-band absolute magnitude of the host galaxy; Col. (7): R-band absolute magnitude of the QSO; Col. (8): references for MR; Col. (9): extended radio power (in units of W Hz-1) at 5 GHz; Col. (10): references for $L_{\rm 5~ GHz}^{\rm ext}$.

REFERENCES - (1) Boyce et al. (1999); (2) Hamilton et al. (2002); (3) Dunlop et al. (2003); (4) Hooper et al. (1997); (5) Boyce et al. (1998); (6) Xu et al. (1999); (7) Rector et al. (1995); (8) Bogers et al. (1994); (9) Aldcroft et al. (1993); (10) Hutchings et al. (1996); (11) White 1992); (12) Lister et al. (1994); (13) Brotherton (1996); (14) Hooper et al. (1996).
a Based on the index between 0.365 and 4.85 GHz (Gregory & Condon 1991; Douglas et al. 1996).
b Based on the index between 4.85 and 8.4 GHz (Gregory & Condon 1991 and Ref. 14).

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