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Table 1.
Number of galaxies observed through each photometric band.
| Instrument | Wavelength | Label | Number of galaxies |
|
|---|---|---|---|---|
| (central) | 3σ detection | Total | ||
| WISE | 3.4 μm | WISE1 | 725 | 751 |
| 4.6 μm | WISE2 | 663 | 739 | |
| 11.6 μm | WISE3 | 554 | 728 | |
| 22.1 μm | WISE4 | 438 | 694 | |
| IRAC | 3.5 μm | IRAC1 | 277 | 292 |
| (Spitzer) | 4.5 μm | IRAC2 | 359 | 390 |
| 5.7 μm | IRAC3 | 100 | 113 | |
| 7.8 μm | IRAC4 | 116 | 130 | |
| MIPS | 23.7 μm | MIPS1 | 125 | 178 |
| (Spitzer) | 71 μm | MIPS2 | 32 | 41 |
| 156 μm | MIPS3 | 18 | 25 | |
| PACS | 70 μm | PACS1 | 108 | 144 |
| (Herschel) | 100 μm | PACS2 | 273 | 456 |
| 160 μm | PACS3 | 296 | 493 | |
| SPIRE | 250 μm | SPIRE1 | 481 | 674 |
| (Herschel) | 350 μm | SPIRE2 | 446 | 658 |
| 500 μm | SPIRE3 | 404 | 634 | |
| IRAS | 60 μm | IRAS3 | 282 | 360 |
| 100 μm | IRAS4 | 391 | 501 | |
| HFI | 350 μm | HFI1 | 217 | 275 |
| (Planck) | 550 μm | HFI2 | 127 | 182 |
| 850 μm | HFI3 | 93 | 125 | |
Notes. During the inference process (Sect. 3.2), the observed fluxes are compared to the SED model integrated within the transmission of these filters, with the appropriate flux convention.
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