Table 1: High spatial resolution observations of the nulear emission of NGC 1068 from radio to infrared frequencies.
Frequency Flux spatial scale Reference
  [Jy] [mas]  
$2.3\times10^{14}$ 0.0084 78 this work
$1.8\times10^{14}$ 0.022 130 this work
$1.4\times10^{14}$ 0.098 78 this work
$1.2\times10^{14}$ $0.32\pm0.03$ 78 this work
$7.9\times10^{13}$ 1.5 700 [1]
$6.7\times10^{13}$ 2.5 162 this work
$3.8\times10^{13}$ 4.23 200 [2]
$3.0\times10^{13}$ 3.33 200 [2]
$2.5\times10^{13}$ 7.1 200 [2]
$1.6\times10^{13}$ 9.6 $290\times180$ [3]
$1.2\times10^{13}$ 9.4 200 [2]
$2.3\times10^{11}$ $0.022\pm0.008$ $1000\times600$ [4]
$1.15\times10^{11}$ $0.023\pm 0.05$ 1400 [4]
$4.3\times10^{10}$ $0.019 \pm 0.003$ 75 [5]
$2.25\times10^{10}$ $0.016 \pm 0.006$ 75 [5]
$8.4\times10^{9}$ $0.0054 \pm 0.0005$ $11.0\times3.7$ [6]
$5.0\times10^{9}$ $0.0091 \pm 0.0008$ $16.6\times11.2$ [6]
$5.0\times10^{9}$ 0.0051 $14\times3$ [7]
$1.7\times10^{9}$ <0.0026 $14\times12$ [7]
$1.4\times10^{9}$ < $6\times10^{-5}$ $16.0\times7.6$ [6]
[1] Marco & Brooks (2003); [2] Bock et al. (2000); [3] Tomono et al. (2001); [4] Krips et al. (2006); [5] Muxlow et al. (1996); [6] Gallimore et al. (2004); [7] Roy et al. (1998).


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