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Table 5.

AGN classification schemes (infrared and X-ray selection).

Infrared
X-ray
Source ID Power law L07 K12 D12 S05 KI KIM WISE L0.5−7 keV
(1) (10) (11) (12) (13) (14) (15) (16) (17) (18)
J123555+620902* 0.96 3.1 × 1044(o)
J123607+620951* 0.86 × × × × × × 8.3 × 1042(o)
J123608+621036* −1.66 4 × 1042(o)
J123618+621541* 0.45 × × × × × × (3.8×1042)
J123620+620844* 1.38 × × × × × × (2.3×1042)
J123621+621708* −0.22 × × × × × (9.5×1042)
J123623+620654* 0.05 × × × × × (2.4×1043)
J123624+621643* 0.71 × × × × × × (3.5×1042)
J123641+621833* 1.06 × × × × × × × 1.1×1042
J123642+621331* −0.76 × × × 6×1042
J123644+621133* 1.38 × × × × × × 1.1×1042
J123646+621405* −0.12 × × × × 1.3 × 1044(o)
J123650+620738* 2.04 5 × 1044(o)
J123653+621444* 1.42 × × × × × × × 1.3 × 1041
J123659+621833* 1.02 5.2 × 1043(o)
J123700+620910* −0.49 × × × - × (1.1×1043)
J123709+620838* 1.35 × × × × × × 3.2×1042
J123714+621826* 1.71 - 2.2×1044
J123715+620823* −0.45 × × 1.8 × 1042(o)
J123716+621512* 1.37 × × × × × × × 3.7 × 1041
J123717+621733* 1.62 1.8 × 1044(o)
J123720+620741 × × (3.0×1042)
J123721+621130 2.9 × 1043(o)
J123726+621129* 0.86 × × × × × × (1.1×1042)
J123649+620439 × 6.1×1040
J123701+622109* 1.5 × × × × × 1.5×1042
J123739+620505 (1.6×1044)
J123751+621919* 1.13 × × × × × (6.0×1042)
J123523+622248 ×
J123510+622202
J123656+615659 1.2 × × × × × ×

R 20% 48% 24% 24% 33% 33% 40% 30% 59%
(5/25) (12/25) (6/25) (6/25) (8/24) (8/24) (8/20) (4/13) (16/28)

Notes. Check-marks or bold-face entries correspond to a positive AGN classification. Entries with a hyphen correspond to sources which are outside the field-of-view of the bands required to classify the object or are not in the redshift range of the classification scheme. Blank entries have multi-wavelength coverage but do no have detections in all bands required. The column headers correspond to: (10) – Infrared power law classification (Alonso-Herrero et al. 2006; Donley et al. 2007). (11) – Lacy et al. (2007). (12) – Kirkpatrick et al. (2012). (13) – Donley et al. (2012). (14) – Stern et al. (2005). (15) – Messias et al. (2012, 2014)Ks+IRAC. (16) – Messias et al. (2012, 2014)Ks+IRAC+MIPS (17) – Stern et al. (2012) WISE classification. (18) – 0.5–7 keV Chandra X-ray luminosities in erg s−1. Those sources denoted with an (o) are classified as obscured by Xue et al. (2016) (i.e., Γ < 1) while bracketed entries correspond to X-ray upper limits.

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