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Fig. 2.
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SPIRE-350 μm flux density distribution of the targets observed with IRAM in this study (solid magenta line: CO-detected, and dashed turquoise line: CO not-detected), and of all SPIRE sources (black line) situated in the PHz fields in the region of the sky visible from the IRAM-30 m telescope site (δ ≳ −2°).
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