Table 1: Number of sources at 0.6<z<0.8 for the different selections applied to the original sample of galaxies selected at 24 $\mu$ m. Each row of the table corresponds to an additional selection applied to the original sample of 623 sources ( from top to bottom). The final sample of LIRGs is described in the last row of the table
selected at 24 $\mu$ m NUV detections

original sample 623 -

one single optical counterpart 558 -

reliable NUV photometry 402 331

LIRGs 190 158

**Table 1:** Number of sources at 0.6<z<0.8 for the different selections applied to the original sample of galaxies selected at 24 $\mu$ m. Each row of the table corresponds to an additional selection applied to the original sample of 623 sources ( *from top to bottom*). The final sample of LIRGs is described in the last row of the table
	selected at 24 $\mu$ m	NUV detections
original sample	623	-
one single optical counterpart	558	-
reliable NUV photometry	402	331
LIRGs	190	158

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