Table 3
Summary of the 3C 326N emission line flux measurements used in this paper.
| Instrument | Line | Rest wavelength | Flux | FWHM | Reference |
| [μm] | [10-18 W m-2] | [km s-1] | |||
|
|
|||||
| IRAM PdBI | CO(1−0) | 2600 | 0.0035 ± 0.0007 | 350 ± 100 | Nesvadba et al. (2011) |
| Herschel/PACS | [CII] | 157.74 | 11.8 ± 1.0 | 372 ± 12 a | This paper |
| Herschel/PACS | [OI] | 63.18 | 6.1 ± 1.3 | 352 ± 31 | Guillard et al. (2014) |
| Spitzer IRSb | H2 0−0 S(1) | 17.1 | 6.9 ± 0.6 | Unresolved | Ogle et al. (2010) |
| Spitzer IRS | PAHc | 7.7 | <6 | Undetected | Ogle et al. (2010) |
| VLT SINFONId | H2 1−0 S(3) | 1.958 | 2.2 ± 0.2 | 594 ± 41 | Nesvadba et al. (2011) |
| VLT SINFONI | Paα | 1.875 | 1.20 ± 0.14 | 516 ± 44 | Nesvadba et al. (2011) |
| SDSSe | Hα | 0.65646 | 9.3 ± 0.5 | 600 ± 30 | Nesvadba et al. (2010) |
| SDSS | Hβ | 0.48627 | 2.4 ± 0.2 | 610 ± 30 | Nesvadba et al. (2010) |
Notes.
Since the line is highly asymmetric, we give a direct measurement of the line width at 50% of the maximum flux.
For more rotational H2 line and PAH measurements, see Ogle et al. (2010).
For more ro-vibrational H2 line and other NIR line measurements, see Nesvadba et al. (2011).
For more optical line measurements, see Nesvadba et al. (2010).
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