Fig. A.1.

Observed SEDs obtained by combining Pan-STARRS, WIRCam, IRAC, SPIRE, SCUBA-2, and ALMA data (filled black circles) and best-fit templates (magenta curves) obtained with EAZY (Brammer et al. 2008) at the annotated photometric redshifts. The blue curve is the best-fit template at the spectroscopic redshift, available only for IDs 3 and 8. The green curve is the best-fit template to the Pan-STARRS-WIRCam-IRAC SED obtained using Hyper−z (Bolzonella et al. 2000) and the stellar population models of Bruzual & Charlot (2003). Single-temperature modified black-body models that fit the FIR-mm SED to within ±1σ are shown as solid purple curves, and dashed red or cyan curves for the warmer and cooler best fits.
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