Table 4.
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Results of 1H 0323+342 blackbody + power-law spectral fit to the stacked spectra.

StateΓkTFbbFplRχ2/dof
T11.74|$^{+0.06}_{-0.06}$|160|$^{+9}_{-9}$|43.9|$^{+3.2}_{-3.2}$|98.2|$^{+4.2}_{-4.1}$|44.8 per cent58.8/64
T21.85|$^{+0.07}_{-0.07}$|162|$^{+17}_{-18}$|9.8|$^{+1.3}_{-1.3}$|43.3|$^{+1.8}_{-1.7}$|22.7 per cent50.3/52
High flux1.89|$^{+0.07}_{-0.07}$|150|$^{+13}_{-14}$|52.3|$^{+6.1}_{-6.0}$|182.3|$^{+8.3}_{-8.0}$|28.7 per cent54.3/53
Low flux1.75|$^{+0.06}_{-0.06}$|170|$^{+40}_{-38}$|4.0|$^{+1.1}_{-1.1}$|41.5|$^{+1.4}_{-1.3}$|9.7 per cent75.7/60
Flat αox1.88|$^{+0.06}_{-0.06}$|151|$^{+13}_{-14}$|47.8|$^{+5.6}_{-5.6}$|179.6|$^{+7.5}_{-7.3}$|26.6 per cent44.2/57
Steep αox1.68|$^{+0.06}_{-0.06}$|171|$^{+15}_{-16}$|9.2|$^{+1.1}_{-1.1}$|41.3|$^{+1.4}_{-1.4}$|22.3 per cent66.5/62
StateΓkTFbbFplRχ2/dof
T11.74|$^{+0.06}_{-0.06}$|160|$^{+9}_{-9}$|43.9|$^{+3.2}_{-3.2}$|98.2|$^{+4.2}_{-4.1}$|44.8 per cent58.8/64
T21.85|$^{+0.07}_{-0.07}$|162|$^{+17}_{-18}$|9.8|$^{+1.3}_{-1.3}$|43.3|$^{+1.8}_{-1.7}$|22.7 per cent50.3/52
High flux1.89|$^{+0.07}_{-0.07}$|150|$^{+13}_{-14}$|52.3|$^{+6.1}_{-6.0}$|182.3|$^{+8.3}_{-8.0}$|28.7 per cent54.3/53
Low flux1.75|$^{+0.06}_{-0.06}$|170|$^{+40}_{-38}$|4.0|$^{+1.1}_{-1.1}$|41.5|$^{+1.4}_{-1.3}$|9.7 per cent75.7/60
Flat αox1.88|$^{+0.06}_{-0.06}$|151|$^{+13}_{-14}$|47.8|$^{+5.6}_{-5.6}$|179.6|$^{+7.5}_{-7.3}$|26.6 per cent44.2/57
Steep αox1.68|$^{+0.06}_{-0.06}$|171|$^{+15}_{-16}$|9.2|$^{+1.1}_{-1.1}$|41.3|$^{+1.4}_{-1.4}$|22.3 per cent66.5/62

Notes. A Galactic absorption of column density of |$N^{\rm Gal}_{\rm H}=1.17\times 10^{21}\rm \, cm^{-2}$| is always included during the fitting. Column 2: Photon index. Column 3: Blackbody temperature in units of eV. Column 4: Flux of the blackbody component in the band 0.3–2 keV in units of 10−13  |$\rm erg\, s^{-1}\,cm^{-2}$|⁠. Column 5: Flux of power-law component in the band 0.3–2 keV in units of 10−13|$\rm erg\, s^{-1}\,cm^{-2}$|⁠. Column 6: Flux ratio of blackbody to power law in the band 0.3–2 keV.  Column 7: χ2 and the dof.

Table 4.
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Results of 1H 0323+342 blackbody + power-law spectral fit to the stacked spectra.

StateΓkTFbbFplRχ2/dof
T11.74|$^{+0.06}_{-0.06}$|160|$^{+9}_{-9}$|43.9|$^{+3.2}_{-3.2}$|98.2|$^{+4.2}_{-4.1}$|44.8 per cent58.8/64
T21.85|$^{+0.07}_{-0.07}$|162|$^{+17}_{-18}$|9.8|$^{+1.3}_{-1.3}$|43.3|$^{+1.8}_{-1.7}$|22.7 per cent50.3/52
High flux1.89|$^{+0.07}_{-0.07}$|150|$^{+13}_{-14}$|52.3|$^{+6.1}_{-6.0}$|182.3|$^{+8.3}_{-8.0}$|28.7 per cent54.3/53
Low flux1.75|$^{+0.06}_{-0.06}$|170|$^{+40}_{-38}$|4.0|$^{+1.1}_{-1.1}$|41.5|$^{+1.4}_{-1.3}$|9.7 per cent75.7/60
Flat αox1.88|$^{+0.06}_{-0.06}$|151|$^{+13}_{-14}$|47.8|$^{+5.6}_{-5.6}$|179.6|$^{+7.5}_{-7.3}$|26.6 per cent44.2/57
Steep αox1.68|$^{+0.06}_{-0.06}$|171|$^{+15}_{-16}$|9.2|$^{+1.1}_{-1.1}$|41.3|$^{+1.4}_{-1.4}$|22.3 per cent66.5/62
StateΓkTFbbFplRχ2/dof
T11.74|$^{+0.06}_{-0.06}$|160|$^{+9}_{-9}$|43.9|$^{+3.2}_{-3.2}$|98.2|$^{+4.2}_{-4.1}$|44.8 per cent58.8/64
T21.85|$^{+0.07}_{-0.07}$|162|$^{+17}_{-18}$|9.8|$^{+1.3}_{-1.3}$|43.3|$^{+1.8}_{-1.7}$|22.7 per cent50.3/52
High flux1.89|$^{+0.07}_{-0.07}$|150|$^{+13}_{-14}$|52.3|$^{+6.1}_{-6.0}$|182.3|$^{+8.3}_{-8.0}$|28.7 per cent54.3/53
Low flux1.75|$^{+0.06}_{-0.06}$|170|$^{+40}_{-38}$|4.0|$^{+1.1}_{-1.1}$|41.5|$^{+1.4}_{-1.3}$|9.7 per cent75.7/60
Flat αox1.88|$^{+0.06}_{-0.06}$|151|$^{+13}_{-14}$|47.8|$^{+5.6}_{-5.6}$|179.6|$^{+7.5}_{-7.3}$|26.6 per cent44.2/57
Steep αox1.68|$^{+0.06}_{-0.06}$|171|$^{+15}_{-16}$|9.2|$^{+1.1}_{-1.1}$|41.3|$^{+1.4}_{-1.4}$|22.3 per cent66.5/62

Notes. A Galactic absorption of column density of |$N^{\rm Gal}_{\rm H}=1.17\times 10^{21}\rm \, cm^{-2}$| is always included during the fitting. Column 2: Photon index. Column 3: Blackbody temperature in units of eV. Column 4: Flux of the blackbody component in the band 0.3–2 keV in units of 10−13  |$\rm erg\, s^{-1}\,cm^{-2}$|⁠. Column 5: Flux of power-law component in the band 0.3–2 keV in units of 10−13|$\rm erg\, s^{-1}\,cm^{-2}$|⁠. Column 6: Flux ratio of blackbody to power law in the band 0.3–2 keV.  Column 7: χ2 and the dof.

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