The SRG/eROSITA diffuse soft X-ray background - I. The local hot bubble in the western Galactic hemisphere

Open Access

Fig. 18

Similar to Fig. 17 but for the spherical harmonics model of l_max = 6. The data were fitted down to 10° from the Galactic plane. We note that the colour bar of the left panel was scaled up to 0.2 keV, identical to Fig. 10 for comparison.

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