Fig. 11.
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Temporal variation of the best-fit spectral parameters of RX J0520.5–6932 from individual NICER observations during the 2024 outburst. The panels show (from top to bottom) the LMC Column density (
) in units of 1021 cm−2, blackbody temperature (kTBB), blackbody radius (RBB) assuming a distance of 50 kpc, emission line centroid energy (Eline), normalization of emission line (×10−3), equivalent width of emission line, photon index (Γ), normalization of powerlaw (×10−2), unabsorbed flux in the 0.5–10 keV range in units of 10−10 erg cm−2 s−1, and reduced χ2 of best-fit, respectively.
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