Table C.1.
Photometry of 3C 326 N. The photometric bands derived from the Sloan Digital Sky Surveys (SDSS) were obtained using a circular aperture with a diameter of 8 arcsec on the SDSS DR18 (Almeida et al. 2023).
| Bands | Flux (mJy) |
|---|---|
| NUV GALEX⋆ | 0.011 ± 0.002 a |
| SDSS u | 0.081 ± 0.017 b |
| SDSS r | 0.430 ± 0.040 b |
| SDSS g | 1.082 ± 0.063 b |
| SDSS i | 1.749 ± 0.080 b |
| SDSS z | 2.371 ± 0.093 b |
| UKIRT J | 2.36 ± 0.06 c |
| UKIRT H | 2.66 ± 0.07 c |
| UKIRT Ks | 2.39 ± 0.06 c |
| Spitzer MIPS 24 μm | 0.52 ± 0.07 d |
| Spitzer MIPS 70 μm | 6.12 ± 0.65 d |
| Herschel PACS 100 μm | 16.7 ± 0.6 d |
| Herschel PACS 160 μm | 15.9 ± 0.6 d |
| Herschel SPIRE 250 μm | 9.0 ± 3.5 d |
Notes. ⋆Ogle et al. (2010) report a NUV AB magnitude of 21.47 (i.e., surface brightness of 1.59 × 10−6 W m−2 sr−1) assuming a diameter area of 5 arcsec. The value is converted into flux density with an uncertainty equal to 20% of the observation. (a) Ogle et al. (2010; b) This work; (c) Lilly & Longair (1984; d) Guillard et al. (2015b)
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