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Table 1.

Summary of the photometric data used for the SED-fitting modeling.

Field λ range Reference Telescope/Instrument Bands
XMM-XXL UV to MIR Georgakakis et al. (2017) and GALEX NUV
Fotopoulou et al. (2016) CFHT u, g, r, i, z
SDSS u, g, r, i, z
VISTA z, Y, J, H, K
Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 μm
Lang et al. (2016) WISE W1, W2, W3, W4
24 − 500 μm Oliver et al. (2012) Spitzer/MIPS 24 μm
Herschel/PACS 70, 100, 160 μm
Herschel/SPIRE 250, 350, 500 μm

CDF-S UV to MIR Hsu et al. (2014) CTIO-Blanco/Mosaic-II U
VLT/VIMOS U
HST/ACS F435W, F606W, F775W, F814W, F850LP
HST/WFC3 F098M, F105W, F125W, F160W
ESO-MPG/WFI UU38BVRI
CTIO-Blanco/Mosaic-II z-band
NTT/SofI H-band
CTIO-Blanco/ISPI J, K
VLT/ISAAC KS
VLT/HAWK-I KS
Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 μm
24 − 160 μm Magnelli et al. (2013) or Spitzer/MIPS 24 μm
Lutz et al. (2011) Herschel/PACS 70, 100, 160 μm
250 − 500 μm Oliver et al. (2012) Herschel/SPIRE 250, 350, 500 μm
> 1000 μm Scholtz et al. (2018) and ALMA Band 7 (800−1100 μm)
ALMA Archive Band 3 (2600−3600 μm)

COSMOS UV to MIR Laigle et al. (2016) GALEX NUV
CFHT/MegaCam u*
Subaru/Suprime-Cam B, V, r, i+, z++,
Subaru/HSC Y
VISTA/VIRCAM Y, J, H, Ks
CFHT/WIRCam H, Ks
Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 μm
24 − 160 μm Lutz et al. (2011) Spitzer/MIPS 24 μm
Herschel/PACS 70, 100, 160 μm
250 − 500 μm Hurley et al. (2017) Herschel/SPIRE 250, 350, 500 μm
> 1000 μm Scholtz et al. (2018) and ALMA Band 7 (800−1100 μm)
ALMA Archive Band 3 (2600−3600 μm)

WISSH UV to MIR Duras et al. (in prep.) SDSS u, g, r, i, z
2MASS J, H, K
WISE W1, W2, W3, W4

Stripe 82X UV to MIR Ananna et al. (2017) SDSS u, g, r, i, z
UKIDSS J, H, K
VISTA J, H, K
Spitzer/IRAC 3.6, 4.5 μm
Lang et al. (2016) WISE W1, W2, W3, W4

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