Table 1.
Broad and intermediate bands (UV to mm) in this work.
| Telescope/Camera | Filter | λc (μm) | Ref. |
|---|---|---|---|
| VLT/VIMOS | U | 0.3759 | (a) |
| R | 0.6481 | ||
| HST/ACS | F435W | 0.4347 | (b) |
| F606W | 0.6033 | ||
| F775W | 0.7730 | ||
| F814W | 0.8143 | ||
| F850LP | 0.9085 | ||
| HST/WFC3 | F105W | 1.0644 | (b) |
| F125W | 1.2561 | ||
| F140W | 1.4064 | ||
| F160W | 1.5463 | ||
| CFHT/WIRCAM | J | 1.2554 | (c) |
| Ks | 2.1630 | ||
| VLT/ISAAC | J | 1.2423 | (d) |
| H | 1.6560 | ||
| Ks | 2.1709 | ||
| VLT/HAWK-I | Ks | 2.1586 | (e) |
| Magellan/FourStar | J1 | 1.0552 | (f) |
| J2 | 1.1472 | ||
| J3 | 1.2819 | ||
| Hs | 1.5564 | ||
| Hl | 1.7038 | ||
| Ks | 2.1599 | ||
| Spitzer/IRAC | CH1 | 3.5763 | (g) |
| CH2 | 4.5289 | ||
| CH3 | 5.7875 | ||
| CH4 | 8.0449 | ||
| Spitzer/MIPS | MIPS | 24 | (h) |
| Herschel/PACS | blue | 70 | (i) |
| green | 100 | ||
| red | 160 | ||
| Herschel/SPIRE | PSW | 250 | |
| PMW | 350 | ||
| PLW | 500 | ||
| ALMA | band 6 | 1130 | (j) |
Notes. These bands are used for the UV-to-MIR and MIR-to-mm SED fitting. From left to right: Telescope and/or instrument, the filter name, the central wavelength of the filters, and the reference for the survey, including the images and catalogs we used. (a)Nonino et al. (2009). (b)HLF program (Whitaker et al. 2019). (c)Hsieh et al. (2012). (d)Retzlaff et al. (2010). (e)Fontana et al. (2014). (f)ZFOURGE program (Straatman et al. 2016). (g)Image: the GREATS program (Stefanon et al. 2021); catalog: this work (see Appendix A). (h)PI: M. Dickinson; catalog: Magnelli et al. (2011). (i)Image: Magnelli et al. (2013) and Elbaz et al. (2011); catalog: T. Wang (priv. comm.) and Elbaz et al. (2011). (j)Image: this work (see Sect. 2.1); catalog (and also image): Gómez-Guijarro et al. (2022a).
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