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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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