Table 22: Synthesis results in terms of flux fractions for NGC 1052 along the minor axis.

Flux fraction at $\lambda $5870 Å
R (arcsec) G1 G2 G3 Y1 Y2 Y3 RHII E(B-V)i
  (%) (%) (%) (%) (%) (%) (%) (mag)
0.00 60.9 $\pm$ 7.8 8.5 $\pm$ 9.2 5.1 $\pm$ 6.1 9.1 $\pm$ 9.0 11.1 $\pm$ 7.4 3.4 $\pm$ 4.6 2.0 $\pm$ 3.2 0.05
2.17 SW 60.7 $\pm$ 3.2 1.7 $\pm$ 2.8 30.3 $\pm$ 5.4 1.0 $\pm$ 2.0 2.5 $\pm$ 3.2 3.7 $\pm$ 3.5 0.0 $\pm$ 0.0 0.02
4.90 SW 69.0 $\pm$ 5.9 7.3 $\pm$ 5.7 5.5 $\pm$ 5.3 3.7 $\pm$ 4.0 9.0 $\pm$ 5.5 2.7 $\pm$ 3.4 2.8 $\pm$ 3.2 0.03
9.41 SW 66.9 $\pm$ 6.1 13.7 $\pm$ 6.6 8.4 $\pm$ 6.3 2.2 $\pm$ 3.1 3.9 $\pm$ 4.1 3.3 $\pm$ 3.9 1.5 $\pm$ 2.5 0.02
2.19 NE 70.3 $\pm$ 7.3 11.2 $\pm$ 7.0 9.7 $\pm$ 6.4 2.4 $\pm$ 3.2 2.3 $\pm$ 3.1 2.7 $\pm$ 3.5 1.4 $\pm$ 2.4 0.05
4.92 NE 57.3 $\pm$ 8.0 19.2 $\pm$ 9.1 2.7 $\pm$ 3.9 4.4 $\pm$ 4.7 9.3 $\pm$ 6.7 2.1 $\pm$ 3.1 5.0 $\pm$ 4.0 0.01
9.43 NE 56.5 $\pm$ 6.6 12.2 $\pm$ 7.4 4.1 $\pm$ 4.5 4.4 $\pm$ 4.5 14.5 $\pm$ 6.8 2.9 $\pm$ 3.9 5.3 $\pm$ 3.9 0.02

Tables notes. Last column: internal reddening, corresponding to the Galactic law.

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