Fig. 9.
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Cumulative resolved and unresolved emission for all objects classes in different surveys, compared with the “Base Max” interstellar emission model from De la Torre Luque et al. (2022) integrated over the survey footprint (in black, labeled “IEM”). The mismatch in the number of objects detectable in the HAWC survey between the top panel and Table 2 is due to the restriction of the footprint (see text).
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