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Table E.4.

Summary of the photometric data used for the SED-fitting modeling described in Appendix D.

Field λ range Reference Telescope/Instrument Bands
CDF-S UV to NIR Merlin et al. (2021) CTIO-Blanco/Mosaic-Iwe U
VLT/VIMOS U, B, R
HST/ACS F435W, F606W, F775W, F814W, F850LP
HST/WFC3 F098M, F105W, F125W, F160W
VLT/HAWK-we KS
3 − 500 μm Shirley et al. (2021) Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 μm
Spitzer/MIPS 24 μm
Herschel/PACS 70, 100, 160 μm
Herschel/SPIRE 250, 350, 500 μm
> 1000 μm Scholtz et al. (2018), ALMA Band 7 (800−1100 μm)
González-López et al. (2020), Band 6 (1100–1400 μm)
Aravena et al. (2020) Band 5 (1400–1800 μm)
and this work Band 4 (1800–2400 μm)
Band 3 (2600−3600 μm)

COSMOS UV to MIR Weaver et al. (2022) CFHT/MegaCam u, u*
HST/ACS F814W
Subaru/HSC g, r, i, z, y
Subaru/Suprime-Cam B, g+, V, r+, i+, z+, z++
VISTA/VIRCAM Y, J, H, Ks
Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 μm
24 − 500 μm a Jin et al. (2018) Spitzer/MIPS 24 μm
Herschel/PACS 70, 100, 160 μm
Herschel/SPIRE 250, 350, 500 μm
> 1000 μm Scholtz et al. (2018), ALMA Band 7 (800−1100 μm)
Circosta et al. (2021) Band 6 (1100–1400 μm)
and this work Band 4 (1800–2400 μm)
Band 3 (2600−3600 μm)

X-UDS UV to FIR Shirley et al. (2021) CFHT/MegaCam u*
Subaru/Suprime r
Subaru/HSC g, i, z, y
UKIDSS J, H, K
VISTA/VIRCAM Ks
Spitzer/IRAC 3.6, 4.5, 5.8, 8.0 μm
Spitzer/MIPS 24 μm
Herschel/PACS 70, 100, 160 μm
Herschel/SPIRE 250, 350, 500 μm
> 1000 μm Scholtz et al. (2018), ALMA Band 7 (800−1100 μm)
and this work Band 6 (1100–1400 μm)
Band 5 (1400–1800 μm)
Band 4 (1800–2400 μm)
Band 3 (2600−3600 μm)

Notes. a The 24 − 500 μm photometry of lid_1565 and cid_72 is collected from Lutz et al. (2011) and Hurley et al. (2017).

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