Table 1.
Overview of the observational data covering the NEP used in this work approximately ordered from long to short wavelengths.
| Telescope | Wavelength | Area | Beam size/PSF | Depth |
|---|---|---|---|---|
| [Catalogue] | [deg2] | [arcsec] | ||
| JCMT-SCUBA-2 | 850 [μm] | 0.6 | 15 | 1.2 mJy beam−1 |
| (Geach et al. 2017) | (1σ) | |||
| Herschel-SPIRE | 250–350–500 [μm] | 9 | 18–25–36 | 9.0–7.5–10.8 [mJy] |
| (Pearson et al. 2017/Pearson et al., in prep.) | (3σ) | |||
| Herschel-PACS | 100–160 [μm] | 0.69 | 7–12 | 4–8 mJy |
| (Pearson et al. 2019) | (3σ) | |||
| Spitzer-MIPS | 24 [μm] | 2 | 6 | 30 μJy |
| (Shirley et al. 2019) | (3σ) | |||
| AKARI-IRC | 2.4–3.2–4.1–7.0–9.0– | 0.69 | 2.9–6.7 | 11–9–10–30–34 |
| (Murata et al. 2013) | 11–15–18–24 [μm] | 57–87–93–256 μJy (5σ) | ||
| AKARI-IRC | 2.4–3.2–4.1–7.0–9.0– | 5.4 | 2.9–6.7 | 15–13–13–57–69 |
| (Kim et al. 2012) | 11–15–18–24 [μm] | 100–144–144–275 μJy (5σ) | ||
| Spitzer-IRAC | 3.6–4.5 [μm] | 7.04 | 1.78 | 1.9–0.79 μJy |
| (Nayyeri et al. 2018) | (1σ) | |||
| WIRCAM/CFHT | Y–J–Ks | 0.69 | 24–23–26 mag [AB] | |
| SuprimeCam/SUBARU | B, V, R, i, z | 0.3 | 0.6–1.2 | ∼25 mag [AB](5σ) |
| MegaCam/CFHT | u–g–r–i–z | 0.69 | 0.84–0.96 | 26–26–26–25–24 mag [AB] (5σ) |
| (Murata et al. 2013) | ||||
| CHFT | u–g–r–i–z | 2 | 0.84–0.96 | 26–26–26–25–24 |
| (Kim et al. 2012) | mag [AB] (5σ) | |||
| SUBARU/HSC | g–r–i–z–Y | 5.4 | 0.6–1.2 | 27.18–26.71–26.10–25.26–24.78 |
| (Oi et al., in prep.) | mag [AB] (5σ) | |||
| GALEX | NUV-FUV | All sky | 4.5–6 | ∼23 |
| (Bianchi 2014) | mag [AB] (5σ) |
Notes. The first column indicates the name of the telescope and the reference corresponding to the catalogue used. The second column indicates the photometric bands considered and the third column shows the area covered. The fourth column corresponds to the beam size of the telescopes, and the depth is shown in the fifth column. All of these catalogues have astrometric errors smaller than 2 arcsec.
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