Table 4.

Best-fitting values for |$\lt 2\rm ~ keV$| X-ray spectral fitting.

ObjectModelΓ0.35-2keVf0.35-2 keVW-stat/DOF
|$\rm (erg~ s^{-1} cm^{-2})$|
IRAS04416+121512.52 ± 0.144.84E-1230.9/36
SDSSJ074352.02+271239.5a11.982.31E-1310.7/11
SDSSJ080131.58+354436.413.51 ± 0.114.19E-1261.9/54
SDSSJ083553.46+055317.113.12 ± 0.113.18E-1236.4/43
SDSSJ084533.28+474934.5a2.362.56E-1315.2/17
SDSSJ093302.68+385228.0a2.274.46E-1319.8/16
SDSSJ100402.61+285535.313.27 ± 0.181.82E-1225.8/26
SDSSJ101000.68+300321.513.10 ± 1.104.08E-146.6/6
SDSSJ075051.72+245409.3a2.394.74E-135.8/6
ObjectModelΓ0.35-2keVf0.35-2 keVW-stat/DOF
|$\rm (erg~ s^{-1} cm^{-2})$|
IRAS04416+121512.52 ± 0.144.84E-1230.9/36
SDSSJ074352.02+271239.5a11.982.31E-1310.7/11
SDSSJ080131.58+354436.413.51 ± 0.114.19E-1261.9/54
SDSSJ083553.46+055317.113.12 ± 0.113.18E-1236.4/43
SDSSJ084533.28+474934.5a2.362.56E-1315.2/17
SDSSJ093302.68+385228.0a2.274.46E-1319.8/16
SDSSJ100402.61+285535.313.27 ± 0.181.82E-1225.8/26
SDSSJ101000.68+300321.513.10 ± 1.104.08E-146.6/6
SDSSJ075051.72+245409.3a2.394.74E-135.8/6

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.

Table 4.

Best-fitting values for |$\lt 2\rm ~ keV$| X-ray spectral fitting.

ObjectModelΓ0.35-2keVf0.35-2 keVW-stat/DOF
|$\rm (erg~ s^{-1} cm^{-2})$|
IRAS04416+121512.52 ± 0.144.84E-1230.9/36
SDSSJ074352.02+271239.5a11.982.31E-1310.7/11
SDSSJ080131.58+354436.413.51 ± 0.114.19E-1261.9/54
SDSSJ083553.46+055317.113.12 ± 0.113.18E-1236.4/43
SDSSJ084533.28+474934.5a2.362.56E-1315.2/17
SDSSJ093302.68+385228.0a2.274.46E-1319.8/16
SDSSJ100402.61+285535.313.27 ± 0.181.82E-1225.8/26
SDSSJ101000.68+300321.513.10 ± 1.104.08E-146.6/6
SDSSJ075051.72+245409.3a2.394.74E-135.8/6
ObjectModelΓ0.35-2keVf0.35-2 keVW-stat/DOF
|$\rm (erg~ s^{-1} cm^{-2})$|
IRAS04416+121512.52 ± 0.144.84E-1230.9/36
SDSSJ074352.02+271239.5a11.982.31E-1310.7/11
SDSSJ080131.58+354436.413.51 ± 0.114.19E-1261.9/54
SDSSJ083553.46+055317.113.12 ± 0.113.18E-1236.4/43
SDSSJ084533.28+474934.5a2.362.56E-1315.2/17
SDSSJ093302.68+385228.0a2.274.46E-1319.8/16
SDSSJ100402.61+285535.313.27 ± 0.181.82E-1225.8/26
SDSSJ101000.68+300321.513.10 ± 1.104.08E-146.6/6
SDSSJ075051.72+245409.3a2.394.74E-135.8/6

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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