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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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