Probabilistic and progressive deblended far-infrared and sub-millimetre point source catalogues - I. Methodology and first application in the COSMOS field

Open Access

Table 2

DLNN performance.

DLNN Model	$\tilde{Δ S}$ $\[\widetilde{\Delta S}\]$	NMAD	MFD
MIPS	0.0000	0.0011	−0.0028
PACS100	−0.0001	0.0096	−0.0110
SPIRE250 (opt. − PACS)	−0.0006	0.0066	−0.0230
SPIRE250 (opt. − MIPS)	−0.0001	0.0240	−0.0063

Notes. Both the median bias $\tilde{Δ S}$ $\[\widetilde{\Delta S}\]$ and the normalised median absolute deviation NMAD are in unit of mJy. The median fractional difference MFD is dimensionless. For the PACS DLNN, we report the metrics measured for the 100 μm band. For the two SPIRE DLNNs (one with optical to MIPS data and one with optical to PACS data), we report the results for the 250 μm band.

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