Fig. 1


Cutout of the SRG/eROSITA all-sky survey image from eRASS1 data. The image shows, among many other sources, the extended X-ray emission from the 24° diameter large Antlia Loop in its upper left quadrant and the emission from the Vela SNR in its lower right. Theemission from the Hoinga SNR in the upper right quadrant of the image is indicated. The image is an Aitoff projection of photons that have been colour-coded according to their energy (red for energies 0.3–0.6 keV, green for 0.6–1 keV, blue for 1–2.3 keV). The image was smoothed with a 10′ FWHM Gaussian filter.

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