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Table 1
The observed data: wavelengths corresponding to the filters’ identification of instrument and survey.
| Filters | Wavelength | Instrument-Survey | Galaxies detected |
|
|
|||
| Mid-IR, IR | |||
| MIPS 1 | 24 μm | MIPS/Spitzer – FIDEL | 181 |
| MIPS 2 | 70 μm | ” | 62 |
|
|
|||
| Near-IR | |||
| IRAC 1 | 3.6 μm | IRAC-GTO Spitzer | 177 |
| IRAC 2 | 4.5 μm | ” | 161 |
| IRAC 3 | 5.8 μm | ” | 177 |
| IRAC 4 | 8.0 μm | ” | 161 |
|
|
|||
| UV – Optical | |||
| U | 0.35 μm | MUSYC | 179 |
| U38 | 0.36 μm | ” | 180 |
| B | 0.46 μm | ” | 181 |
| V | 0.54 μm | ” | 181 |
| R | 0.65 μm | ” | 181 |
| I | 0.87 μm | ” | 181 |
| z | 0.90 μm | ” | 181 |
| J | 1.2 μm | ” | 180 |
| H | 1.6 μm | ” | 155 |
| K | 2.1 μm | ” | 181 |
|
|
|||
| UV | |||
| NUV | 2310 Å | GALEX-DIS | 150 |
Notes. Our sample contains 181 galaxies, of which 62 are detected at 70 μm.
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