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Fig. 19.
Distribution of the candidate emitters in the 10 × 10 sq. deg box containing the Heart and Soul nebulae at respectively ℓ ≃ 135° and ℓ ≃ 138°, in the Perseus Arm. High-confidence emitters selected with excess greater than 5σ are in red. More marginal candidates with excesses of between 3 and 5σ are in black.
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