Figure 5 - A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058

Figure 5. X-ray spectra of the PWN (crosses; 1-20 keV) extracted within an R 3 = ¢ circle, and those of the pulsar (empty circles; 1-30 keV). The best-fit instrumental Gaussian lines for the PWN spectra measured by XMM-Newton are presented in dashed black (MOS1) and red (MOS2) lines in the top panel. The pulsar spectrum measured by Chandra (cyan circles in the top panel) includes both the pulsed and off-pulse components, and those measured by NuSTAR are only for the pulsed component (blue and green circles). The bottom panel shows residuals after subtracting the best-fit power-law and instrumental Gaussian models.

X-ray spectra of the PWN (crosses; 1-20 keV) extracted within an R 3 = ¢ circle, and those of the pulsar (empty circles; 1-30 keV). The best-fit instrumental Gaussian lines for the PWN spectra measured by XMM-Newton are presented in dashed black (MOS1) and red (MOS2) lines in the top panel. The pulsar spectrum measured by Chandra (cyan circles in the top panel) includes both the pulsed and off-pulse components, and those measured by NuSTAR are only for the pulsed component (blue and green circles). The bottom panel shows residuals after subtracting the best-fit power-law and instrumental Gaussian models.

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Reference

A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058 - Scientific Figure on ResearchGate. Available from: https://www.researchgate.net/figure/ray-spectra-of-the-PWN-crosses-1-20-keV-extracted-within-an-R-3-circle-and-those_fig3_369254667 [accessed 21 May 2025]

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Figure 5. X-ray spectra of the PWN (crosses; 1-20 keV) extracted within an R 3 = ¢ circle, and those of the pulsar (empty circles; 1-30 keV). The best-fit instrumental Gaussian lines for the PWN spectra measured by XMM-Newton are presented in dashed black (MOS1) and red (MOS2) lines in the top panel. The pulsar spectrum measured by Chandra (cyan circles in the top panel) includes both the pulsed and off-pulse components, and those measured by NuSTAR are only for the pulsed component (blue and green circles). The bottom panel shows residuals after subtracting the best-fit power-law and instrumental Gaussian models.

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<a href="https://www.researchgate.net/figure/ray-spectra-of-the-PWN-crosses-1-20-keV-extracted-within-an-R-3-circle-and-those_fig3_369254667"><img src="https://www.researchgate.net/publication/369254667/figure/fig3/AS:11431281127003412@1678895958873/ray-spectra-of-the-PWN-crosses-1-20-keV-extracted-within-an-R-3-circle-and-those.png" alt="X-ray spectra of the PWN (crosses; 1-20 keV) extracted within an R 3 = ¢ circle, and those of the pulsar (empty circles; 1-30 keV). The best-fit instrumental Gaussian lines for the PWN spectra measured by XMM-Newton are presented in dashed black (MOS1) and red (MOS2) lines in the top panel. The pulsar spectrum measured by Chandra (cyan circles in the top panel) includes both the pulsed and off-pulse components, and those measured by NuSTAR are only for the pulsed component (blue and green circles). The bottom panel shows residuals after subtracting the best-fit power-law and instrumental Gaussian models."/></a>