Table C.1.
An overview of the used data sets representing parts of the whole electromagnetic spectrum.
| Survey | Domain | λ | Δλ | res | nside | pub | Noise | Sources | Flux | Background | Coverage |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Haslam | Radio | 408 MHz | — | 56′0 | 512 | 2014 | ✔ | ✔ | ✔ | ✖ | 100% |
| HI4PI | Radio | 21 cm → NHI | 100 MHz 8 MHz | 16′2 | 1024 | 2016 | ✔ | ✖ | ✔ | ✖ | 100% |
| Stockert, Villa Elisa | Radio | 1420 MHz 1435 MHz 1420 MHz | 18 MHz 14 MHz 13 MHz | 35′4 | 512 | — | ✔ | ✖ | ✔ | ✖ | 100% |
| Planck LFI | Microwave | 30 GHz 44 GHz 70 GHz | Δν/ν = 0.2 | 24′0 | 1024 | 2015 | ✔ | ✖ | ✔ | ✔ | 100% |
| Planck HFI | Microwave | 100 GHz 143 GHz 217 GHz 353 GHz 545 GHz 857 GHz | Δν/ν = 0.3 | 5′5 | 2048 | 2015 | ✔ | ✖ | ✔ | ✔ | 100% |
| Planck CO | Microwave | 115.3 GHz | — | 15′ | 2048 | 2015 | ✔ | ✖ | ✔ | ✔ | 100% |
| AKARI | FIR | 65 μm 90 μm 140 μm 160 μm |
30 μm 50 μm 70 μm 40 μm | 1′3 | 4096 | 2015 | ✔ | ✔ | ✔ | ✔ | >99% |
| IRIS | IR | 12 μm 25 μm 60 μm 100 μm |
6.5 μm 11.0 μm 40.0 μm 37.0 μm | 4′0 | 1024 | 2006 | ✖ | ✖ | ✔ | ✔ | 98% |
| Finkbeiner | Hα | 656.3 nm | 1.7 nm 3.2 nm 4.0 nm | 6′0 | 512 | 2003 | ✖ | ✖ | ✔ | ✖ | 100% |
| ROSAT | X-ray | 0.197 keV 0.212 keV 0.725 keV 0.885 keV 1.145 keV 1.545 keV | 0.174 keV 0.144 keV 0.570 keV 0.650 keV 0.830 keV 0.990 keV | 120′0 | 512 | 2015 | ✖ | ✖ | ✔ | ✔ | 98% |
| Fermi | γ-ray | 0.85 GeV 1.70 GeV 3.40 GeV 6.79 GeV 13.58 GeV 27.15 GeV 54.31 GeV 108.61 GeV 217.22 GeV | 0.6 GeV 1.2 GeV 2.4 GeV 4.8 GeV 9.6 GeV 19.2 GeV 38.4 GeV 76.8 GeV 153.6 GeV | — | 128 | 2015 | ✔ | ✔ | ✔ | ✔ | 100% |
| Fermi | Hadronic, Leptonic | — | — | — | 128 | 2015 | ✔ | ✔ | ✔ | ✔ | <90% |
Notes. Unfilled gaps mean that the effect is not relevant for the survey. λ stands for central wavelength or frequency, Δλ stands for bandwidth, res is short for resolution of the instrument (not the resolution defined by the nside), nside is defining the actual resolution, pub is short for the year of publication; further it is stated whether the data is noise corrected and therefore destriped, partly point and extragalactic source removed, flux calibrated, and background corrected or not; coverage stands for the total all-sky coverage.
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