Fig. 7.
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Comparison between SDSS J095909.51+460014.3 and other γ-NLS1s. K-corrections for the luminosities have been applied. Luminosity of the target is based on the analysis of the 15-month Fermi-LAT data. For other sources, each luminosity value is calculated from energy flux of the time bin with the highest flux level in archival yearly bin light curve (Abdollahi et al. 2022).
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