Table 2: Table of observations. For each galaxy, the slit position angle and exposure time is shown.
  1 $^{\prime\prime}$ Slit 4 $^{\prime\prime}$ Slit  
Galaxy PA $T_{\rm exp}$ PA $T_{\rm exp}$ Date
  (deg) (s) (deg) (s)  
3C 20 125 3600 ... ... 11 Sep. 02
3C 28 59 2400 ... ... 11 Sep. 02
3C 31 144 2400 ... ... 10 Sep. 02
3C 33 146 2400 ... ... 10 Sep. 02
3C 35 111 2400 23 900 10 Sep. 02
3C 66B 135 1200 ... ... 10 Sep. 02
3C 76.1 135 2400 130 900 12 Sep. 02
3C 83.1Ba 166 1800 96 2400 12 Sep. 02
3C 98 150 2400 ... ... 12 Sep. 02
3C 388 71 2400 71 900 11 Sep. 02
3C 381 154 3600 ... ... 11 Sep. 02
3C 386b 12 2400 12 1800 10 Sep. 02
3C 401 0 3600 0 1200 11 Sep. 02
3C 433 66 2400 ... ... 11 Sep. 02
3C 442A 131 2400 57 900 12 Sep. 02
3C 449 1 2400 8 900 10 Sep. 02
3C 452 0 2400 ... ... 12 Sep. 02
3C 465 30 1800 121 900 12 Sep. 02
4C 11.71 326 2400 53 900 10 Sep. 02
4C 12.03 17 2400 17 900 11 Sep. 02
4C 35.40 84 2400 133 1200 12 Sep. 02
a Confused with a star 3 $^{\prime\prime}$ away from the nucleus (de Koff et al. 2000; Poulain et al. 1992).
b A star is superposed on the galaxy nucleus.

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