Object . | Model . | Γ0.35-2keV . | f0.35-2 keV . | W-stat/DOF . |
---|---|---|---|---|
. | . | . | |$\rm (erg~ s^{-1} cm^{-2})$| . | . |
IRAS04416+1215 | 1 | 2.52 ± 0.14 | 4.84E-12 | 30.9/36 |
SDSSJ074352.02+271239.5a | – | 11.98 | 2.31E-13 | 10.7/11 |
SDSSJ080131.58+354436.4 | 1 | 3.51 ± 0.11 | 4.19E-12 | 61.9/54 |
SDSSJ083553.46+055317.1 | 1 | 3.12 ± 0.11 | 3.18E-12 | 36.4/43 |
SDSSJ084533.28+474934.5a | – | 2.36 | 2.56E-13 | 15.2/17 |
SDSSJ093302.68+385228.0a | – | 2.27 | 4.46E-13 | 19.8/16 |
SDSSJ100402.61+285535.3 | 1 | 3.27 ± 0.18 | 1.82E-12 | 25.8/26 |
SDSSJ101000.68+300321.5 | 1 | 3.10 ± 1.10 | 4.08E-14 | 6.6/6 |
SDSSJ075051.72+245409.3a | – | 2.39 | 4.74E-13 | 5.8/6 |
Object . | Model . | Γ0.35-2keV . | f0.35-2 keV . | W-stat/DOF . |
---|---|---|---|---|
. | . | . | |$\rm (erg~ s^{-1} cm^{-2})$| . | . |
IRAS04416+1215 | 1 | 2.52 ± 0.14 | 4.84E-12 | 30.9/36 |
SDSSJ074352.02+271239.5a | – | 11.98 | 2.31E-13 | 10.7/11 |
SDSSJ080131.58+354436.4 | 1 | 3.51 ± 0.11 | 4.19E-12 | 61.9/54 |
SDSSJ083553.46+055317.1 | 1 | 3.12 ± 0.11 | 3.18E-12 | 36.4/43 |
SDSSJ084533.28+474934.5a | – | 2.36 | 2.56E-13 | 15.2/17 |
SDSSJ093302.68+385228.0a | – | 2.27 | 4.46E-13 | 19.8/16 |
SDSSJ100402.61+285535.3 | 1 | 3.27 ± 0.18 | 1.82E-12 | 25.8/26 |
SDSSJ101000.68+300321.5 | 1 | 3.10 ± 1.10 | 4.08E-14 | 6.6/6 |
SDSSJ075051.72+245409.3a | – | 2.39 | 4.74E-13 | 5.8/6 |
Note. aFor these targets extending 2–8 keV Galactic-absorbed power-law model (see Table 3) to |$\lt 2\rm ~ keV$| energies gives the best-fitting results.
Object . | Model . | Γ0.35-2keV . | f0.35-2 keV . | W-stat/DOF . |
---|---|---|---|---|
. | . | . | |$\rm (erg~ s^{-1} cm^{-2})$| . | . |
IRAS04416+1215 | 1 | 2.52 ± 0.14 | 4.84E-12 | 30.9/36 |
SDSSJ074352.02+271239.5a | – | 11.98 | 2.31E-13 | 10.7/11 |
SDSSJ080131.58+354436.4 | 1 | 3.51 ± 0.11 | 4.19E-12 | 61.9/54 |
SDSSJ083553.46+055317.1 | 1 | 3.12 ± 0.11 | 3.18E-12 | 36.4/43 |
SDSSJ084533.28+474934.5a | – | 2.36 | 2.56E-13 | 15.2/17 |
SDSSJ093302.68+385228.0a | – | 2.27 | 4.46E-13 | 19.8/16 |
SDSSJ100402.61+285535.3 | 1 | 3.27 ± 0.18 | 1.82E-12 | 25.8/26 |
SDSSJ101000.68+300321.5 | 1 | 3.10 ± 1.10 | 4.08E-14 | 6.6/6 |
SDSSJ075051.72+245409.3a | – | 2.39 | 4.74E-13 | 5.8/6 |
Object . | Model . | Γ0.35-2keV . | f0.35-2 keV . | W-stat/DOF . |
---|---|---|---|---|
. | . | . | |$\rm (erg~ s^{-1} cm^{-2})$| . | . |
IRAS04416+1215 | 1 | 2.52 ± 0.14 | 4.84E-12 | 30.9/36 |
SDSSJ074352.02+271239.5a | – | 11.98 | 2.31E-13 | 10.7/11 |
SDSSJ080131.58+354436.4 | 1 | 3.51 ± 0.11 | 4.19E-12 | 61.9/54 |
SDSSJ083553.46+055317.1 | 1 | 3.12 ± 0.11 | 3.18E-12 | 36.4/43 |
SDSSJ084533.28+474934.5a | – | 2.36 | 2.56E-13 | 15.2/17 |
SDSSJ093302.68+385228.0a | – | 2.27 | 4.46E-13 | 19.8/16 |
SDSSJ100402.61+285535.3 | 1 | 3.27 ± 0.18 | 1.82E-12 | 25.8/26 |
SDSSJ101000.68+300321.5 | 1 | 3.10 ± 1.10 | 4.08E-14 | 6.6/6 |
SDSSJ075051.72+245409.3a | – | 2.39 | 4.74E-13 | 5.8/6 |
Note. aFor these targets extending 2–8 keV Galactic-absorbed power-law model (see Table 3) to |$\lt 2\rm ~ keV$| energies gives the best-fitting results.
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