Extended Data Fig. 5: Chandra spectra (with relative extraction regions) used to derive the physical properties of the chimneys. | Nature

Extended Data Fig. 5: Chandra spectra (with relative extraction regions) used to derive the physical properties of the chimneys.

From: An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre

Extended Data Fig. 5

a, b, Chandra spectra used to derive the latitudinal profiles at l = 0° and shown in Fig. 2 for the southern (a) and northern (b) sides, respectively. c, XMM-Newton 1.5–2.6 keV emission map in greyscale, showing the extraction areas of the Chandra spectra used to derive the latitudinal profiles at l = 0°, with colours corresponding to those of the spectra. The areas at l ≈ −0.7° indicate the extraction regions of the spectra used to derive the grey constraints in Fig. 2. d, e, XMM-Newton spectra used to derive the latitudinal profiles of the diffuse emission in Fig. 2. The error bars represent 1σ.