Table 5
High-τ 9.7 μm sources not included in our sample because of a high PAH EW.
| Name | α | δ | z | τ | PAH EW | log [L6] | log [LX] | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |
|
|
||||||||
| GN_IRS-4 | 12:36:53.4 | +62:11:39 | 1.272 | 1.12 | 0.67 | 11.40 | 41.8 | |
| GN_IRS-11 | 12:36:21.3 | +62:17:08 | 1.9921 | 1.55 | 1.18 | 11.41 | <42.8 | |
| GN_IRS-13 | 12:37:34.5 | +62:17:23 | 0.642 | 1.37 | 0.48 | 11.27 | 41.3 | |
| GN_IRS-14 | 12:36:22.5 | +62:15:44 | 0.6392 | 3.00 | 0.63 | 10.39 | 41.4 | |
| GN_IRS-15 | 12:37:11.4 | +62:13:31 | 1.992 | 1.09 | 0.78 | 10.74 | 42.8 | |
| GN_IRS-16 | 12:36:37.0 | +62:08:52 | 2.022 | 3.97 | 0.57 | 11.27 | 42.1 | |
| GN_IRS-20 | 12:36:03.2 | +62:11:10 | 0.642 | 2.32 | 0.60 | 10.68 | 41.5 | |
| GN_IRS-21 | 12:36:18.3 | +62:15:50 | 2.002 | 1.96 | 0.66 | 11.19 | 42.4 | |
| FLS-283 | 17:14:58.3 | +59:24:11 | 0.942 | 1.12 | 0.68 | 11.46 | <43.1 | |
Notes. The columns are: (1) Name; (2), (3) Equatorial Spitzer coordinates; (4) Redshift: (5) optical depth at 9.7 μm. (6) PAH equivalent-width at 6.2 μm, in units of μm (except in the case of FLS-283 where the 11.3 μm EW is quoted); (7) Logarithm of the νLν monochromatic luminosity at 6 μm in units of solar luminosity as derived by IRS spectroscopy; (8) X-ray luminosity (uncorrected for obscuration) in the 2−10 keV band in units erg s-1.
IRS from Pope et al. (2008), Murphy et al. (2009) in the case of GOODS or Sajina et al. (2007) in the case of FLS;
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