Table A.1.
Emission line fluxes of the different components (and sub-components) of the system, in units of [×10−18 erg s−1 cm−2].
region | [O II] λ3726 | [O II] λ3729 | Hγ | Hβ | [O III] λ5007 | [O I] λ6300 | Hα | [N II] λ6584 | [S II] λ6716 | [S II] λ6731 | |
---|---|---|---|---|---|---|---|---|---|---|---|
main | 180.7 ± 1.9 | 127.3 ± 0.8 | 45.2 ± 0.4 | 106.8 ± 0.4 | 227.6 ± 0.4 | 7.6 ± 0.5 | 305.3 ± 0.8 | 78.6 ± 0.5 | 28.1 ± 0.7 | 20.9 ± 0.3 | |
main n | 77.9 ± 1.7 | 60.9 ± 0.9 | 28.4 ± 0.4 | 59.6 ± 0.6 | 125.8 ± 0.6 | 5.1 ± 0.4 | 170.3 ± 1.2 | 43.1 ± 0.7 | 14.6 ± 0.6 | 11.0 ± 0.4 | |
main b | 316.1 ± 4.0 | 134.0 ± 1.4 | 11.2 ± 0.6 | 89.7 ± 1.1 | 197.5 ± 1.8 | 3.1 ± 0.5 | 256.4 ± 4.0 | 63.8 ± 1.7 | 26.7 ± 1.1 | 21.1 ± 0.8 | |
south | 81.9 ± 1.6 | 60.1 ± 0.7 | 21.3 ± 0.3 | 45.0 ± 0.3 | 125.0 ± 0.4 | 4.5 ± 0.4 | 128.6 ± 0.6 | 18.8 ± 0.4 | 13.2 ± 0.7 | 10.7 ± 0.3 | |
north | 189.8 ± 1.0 | 210.9 ± 0.5 | 42.1 ± 0.3 | 63.2 ± 0.2 | 202.5 ± 0.3 | 2.5 ± 0.3 | 180.7 ± 0.4 | 29.2 ± 0.3 | 20.9 ± 0.4 | 15.7 ± 0.2 | |
s1 | 8.7 ± 1.0 | 5.7 ± 0.4 | 2.1 ± 0.2 | 7.0 ± 0.2 | 20.4 ± 0.3 | 0.6 ± 0.2 | 20.0 ± 0.4 | 2.1 ± 0.3 | 1.6 ± 0.3 | 1.8 ± 0.2 | |
s2 | 23.4 ± 0.5 | 19.6 ± 0.2 | 5.0 ± 0.1 | 11.5 ± 0.1 | 31.2 ± 0.1 | 1.3 ± 0.1 | 32.9 ± 0.2 | 6.0 ± 0.1 | 3.4 ± 0.2 | 2.8 ± 0.1 | |
s3 | 30.8 ± 0.4 | 24.2 ± 0.2 | 9.3 ± 0.1 | 18.0 ± 0.1 | 54.6 ± 0.1 | 1.7 ± 0.1 | 51.5 ± 0.2 | 6.9 ± 0.1 | 4.9 ± 0.1 | 3.5 ± 0.1 | |
n1 | 12.0 ± 0.2 | 10.2 ± 0.1 | 2.0 ± 0.1 | 7.2 ± 0.1 | 17.6 ± 0.1 | 0.3 ± 0.1 | 20.5 ± 0.1 | 2.6 ± 0.1 | 1.8 ± 0.1 | 1.4 ± 0.1 | |
n2 | 24.5 ± 0.2 | 21.4 ± 0.1 | 4.1 ± 0.1 | 7.5 ± 0.1 | 27.2 ± 0.1 | 0.9 ± 0.1 | 21.5 ± 0.1 | 3.8 ± 0.1 | 2.1 ± 0.1 | 1.8 ± 0.1 | |
n3 | 99.2 ± 0.4 | 79.1 ± 0.2 | 31.3 ± 0.1 | 16.2 ± 0.1 | 78.8 ± 0.1 | 1.6 ± 0.1 | 46.2 ± 0.1 | 4.3 ± 0.1 | 3.7 ± 0.1 | 3.3 ± 0.1 | |
c | 6.2 ± 0.2 | 5.6 ± 0.1 | 1.4 ± 0.1 | 3.5 ± 0.1 | 8.2 ± 0.1 | 0.5 ± 0.1 | 10.0 ± 0.1 | 2.2 ± 0.1 | 0.7 ± 0.1 | 0.6 ± 0.1 |
Notes. Fluxes of the different components identified in Fig. 1. For the main galaxy, we report the fluxes obtained with one Gaussian component model (main) and the fluxes obtained with a two-component model (narrow (main n) and broad (main b) components). The label ‘main n’ and ‘main b’ refer to the narrow and broad component of the two-component model, respectively. For the other regions, the fluxes have been obtained with the one-component model fit. Fluxes have been corrected for obscuration using a Cardelli et al. (1989) attenuation law as is described in Sec. 5.2.1.
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