Table 1
Results from the measurements described in Sect. 3.2 for the apertures defined in the K-band image.
| Aperture | Name | Position | K flux density | Brγ flux | Slope | EW(CO) |
|
|
||||||
| 0 | N1 | (–0.57; 7.66) | 4.61e-01 ± 5.53e-03 | 1.38e-17 ± 7.80e-18 | 1.02 ± 0.05 | 21.7 ± 2.2 |
| 1 | – | (–0.03; 7.03) | 1.89e-02 ± 2.10e-03 | 6.67e-16 ± 6.63e-18 | 1.01 ± 0.10 | 17.7 ± 3.8 |
| 2 | – | (–0.03; 8.03) | 5.83e-02 ± 5.17e-03 | 1.40e-17 ± 4.81e-18 | 1.05 ± 0.07 | 23.7 ± 3.2 |
| 5 | – | (0.16; 6.22) | 2.57e-02 ± 7.29e-04 | 1.28e-16 ± 3.73e-18 | 1.41 ± 0.15 | < 11.7 |
| 6 | M4-2 | (0.33; 7.33) | 6.74e-02 ± 1.95e-03 | 6.68e-16 ± 6.69e-18 | 1.12 ± 0.06 | 15.9 ± 3.0 |
| 10 | M4 | (0.41; 7.07) | 7.98e-02 ± 2.02e-03 | 6.68e-16 ± 6.60e-18 | 1.46 ± 0.07 | < 4.7 |
| 12 | – | (1.28; 7.54) | 2.04e-02 ± 8.74e-04 | 7.51e-18 ± 4.48e-18 | 1.19 ± 0.16 | 20.6 ± 6.3 |
| 14 | – | (2.01; 9.21) | 4.42e-02 ± 1.33e-03 | 5.45e-17 ± 5.39e-18 | 1.15 ± 0.10 | 14.5 ± 4.4 |
| 16 | M5-4 | (2.56; 9.96) | 2.11e-01 ± 2.14e-03 | 1.56e-15 ± 1.92e-17 | 1.20 ± 0.10 | 8.4 ± 3.4 |
| 17 | – | (2.60;10.76) | 4.89e-02 ± 2.50e-03 | 3.02e-17 ± 1.14e-17 | 1.00 ± 0.10 | 15.8 ± 3.8 |
| 19 | M5 | (2.81; 9.79) | 2.10e-01 ± 2.24e-03 | 1.57e-15 ± 1.84e-17 | 1.16 ± 0.05 | < 2.8 |
| 20 | M5-2 | (2.88;10.08) | 2.03e-01 ± 2.09e-03 | 1.54e-15 ± 1.98e-17 | 1.14 ± 0.06 | 4.3 ± 2.8 |
| 22 | M5-3 | (3.13; 9.90) | 2.10e-01 ± 2.26e-03 | 1.59e-15 ± 1.88e-17 | 1.15 ± 0.10 | < 9.0 |
| 24 | – | (3.64; 7.26) | 3.33e-02 ± 3.34e-03 | 2.93e-17 ± 5.55e-18 | 1.18 ± 0.14 | 25.7 ± 5.7 |
| 25 | – | (3.93; 8.06) | 2.96e-02 ± 2.64e-03 | 3.76e-17 ± 3.41e-18 | 1.07 ± 0.18 | 10.4 ± 7.8 |
| 26 | – | (3.94; 5.57) | 2.47e-01 ± 5.24e-03 | 2.01e-17 ± 2.39e-18 | 1.04 ± 0.04 | 20.4 ± 2.3 |
| 27 | N2 | (3.97; 5.57) | 2.47e-01 ± 5.24e-03 | 1.19e-17 ± 2.39e-18 | 0.99 ± 0.05 | 21.1 ± 2.3 |
| 30 | – | (4.77; 5.66) | 7.05e-02 ± 3.92e-03 | 2.60e-18 ± 3.12e-18 | 0.92 ± 0.09 | 18.5 ± 4.0 |
| 32 | M6 | (4.78; 6.94) | 2.60e-01 ± 1.40e-03 | 2.23e-15 ± 1.70e-17 | 1.68 ± 0.04 | < 1.7 |
Notes. The aperture number is defined in Fig. 3 and the corresponding name is given in the second column when appropriate. The positions of the apertures are (Δ(RA); Δ(Dec)) in arcsec with respect to the position of the AGN in the MIR (see text). The K-band flux density is mJy. The Brγ flux is in erg s-1 cm-2. These two fluxes are background-subtracted fluxes measured on the reconstructed images, through “large” apertures as defined at the end of Sect. 3.2 (aperture radius 0.2′′, and background between 0.2′′ and 0.6′′). The slope is defined in the last paragraph of Sect. 3.2. The equivalent width of the CO absorption band EW(CO) is measured through the small apertures following the procedure defined in Sect. 3.2 and is given in Å.
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