Table 1
Different filters and instruments used in each field.
| ELAIS-N1 | Boötes | Lockman hole |
|---|---|---|
| (~7.15 deg2) | (~10.73 deg2) | (~9.5 deg2) |
| DIS FUV (26.3 [mag]) | DIS FUV (26.3 [mag]) | DIS FUV (26.3 [mag]) |
| DIS NUV (26.7 [mag]) | DIS NUV (26.7 [mag]) | DIS NUV (26.7 [mag]) |
| SpARCS u (25.4 [mag]) | SpARCS u (25.9 [mag]) | SpARCS u (25.5 [mag]) |
| PanSTARRS g (25.5 [mag]) | – | SpARCS g (25.8 [mag]) |
| PanSTARRS r (25.2 [mag]) | NDWFS R (25.2 [mag]) | SpARCS r (25.1 [mag]) |
| PanSTARRS i (25.0 [mag]) | NDWFS I (24.6 [mag]) | RCSLenS i (23.8 [mag]) |
| PanSTARRS z (24.6 [mag]) | zBoötes z (23.4 [mag]) | SpARCS z (23.5 [mag]) |
| PanSTARRS y (23.4 [mag]) | LBT y (23.4 [mag]) | – |
| UKIDSS-DXS J (23.2 [mag]) | NEWFIRM J (23.1 [mag]) | UKIDSS-DXS J (23.4 [mag]) |
| – | NEWFIRM H (22.5 [mag]) | – |
| UKIDSS-DXS K (22.7 [mag]) | NEWFIRM K (20.2 [mag]) | UKIDSS-DXS K (22.8 [mag]) |
| SWIRE ch1 (23.4 [mag]) | SDWFS ch1 (23.3 [mag]) | SWIRE ch1 (23.4 [mag]) |
| SWIRE ch2 (22.9 [mag]) | SDWFS ch2 (23.1 [mag]) | SWIRE ch2 (22.9 [mag]) |
| SWIRE ch3 (21.2 [mag]) | SDWFS ch3 (21.6 [mag]) | SWIRE ch3 (21.2 [mag]) |
| SWIRE ch4 (21.3 [mag]) | SDWFS ch4 (21.6 [mag]) | SWIRE ch4 (21.2 [mag]) |
| MIPS24 (20 [μJy]) | MIPS24 (20 μJy]) | MIPS24 (20 μJy]) |
| PACS100 (12.5 [mJy]) | PACS100 (12.5 [mJy]) | PACS100 (12.5 [mJy]) |
| PACS160 (17.5 [mJy]) | PACS160 (17.5 [mJy]) | PACS160 (17.5 [mJy]) |
| SPIRE250 (4 [mJy]) | SPIRE250 (5 [mJy]) | SPIRE250 (4 [mJy]) |
| SPIRE350 (4 [mJy]) | SPIRE350 (5 [mJy]) | SPIRE350 (4 [mJy]) |
| SPIRE500 (6 [mJy]) | SPIRE500 (10 [mJy]) | SPIRE500 (6 [mJy]) |
| LoTSS (20 [μJy]) | LoTSS (30 [μJy]) | LoTSS (23 μJy]) |
Notes. The 3σ depths in AB magnitudes are provided for the FUV to IRAC ch4 bands in brackets. These depths were estimated using variances from empty 3" apertures. For the MIPS, PACS, and SPIRE bands, the limits at which fluxes can still be accurately deblended are given (McCheyne et al. 2022). For the radio data, the rms sensitivity is given.
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