Fig. 1.
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Transmission curves of the photometric bands used to derive galaxy properties (left: UV to NIR) and infrared luminosities (right: Spitzer/MIPS + Herschel/PACS-SPIRE) for the calibration of the IRX. Transmission curves are arbitrarily scaled to one. Two spectra of SFGs, without dust (blue) and with dust (red), are shown at z = 0, 0.5, 1, 1.5, 2.
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