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Table 2

Global properties of the eRASS1 broadband map of the diffuse emission.

Energy band (keV) (1) FWC count rate (ct s−1 deg−2) (2) FWC flux (10−7 erg s−1 deg−2 cm−2 keV−1) (3) Vignette coef. (4)
R45 (0.44–1.21) 1.720 0.0170 0.558
R67 (0.73–2.04) 2.810 0.0269 0.541
0.2–0.4 0.659 0.0095 0.543
0.4–0.6 0.527 0.0119 0.550
0.6–1.0 0.890 0.0166 0.562
1.0–2.3 2.713 0.0311 0.526
2.3–5.0 6.750 0.0600 0.413
Energy band (keV) ECF5e20 (1011 ct cm−2 erg−1) (5) Count rateavg. (ct s−1 deg−2) (6) Surface brightnessavg. (10−11 erg s−1 deg−2 cm−2 keV−1) (7) Total fluxest. (10−7 erg s−1 cm−2 keV−1) (8)
R45 (0.44–1.21) 9.51 10.75 ± 0.51 1.47 ± 0.07 3.03 ± 0.14
R67 (0.73–2.04) 8.13 7.40 ± 0.45 0.69 ± 0.04 1.43 ± 0.08
0.2–0.4 6.06 1.79 ± 0.14 1.45 ± 0.09 2.99 ± 0.18
0.4–0.6 8.69 3.20 ± 0.17 1.85 ± 0.08 3.82 ± 0.16
0.6–1.0 9.84 4.85 ± 0.20 1.24 ± 0.03 2.57 ± 0.06
1.0–2.3 6.51 3.83 ± 0.22 0.46 ± 0.02 0.94 ± 0.04
2.3–5.0 0.82 1.02 ± 0.25 0.55 ± 0.09 1.17 ± 0.19

Notes. All numbers are computed for the western sky (180 < l < 360, −90 > b < 90). Columns: (1) Energy band. (2) The FWC count rate (i.e., instrumental background). (3) FWC flux. (4) Vignette coefficient. (5) ECF in units of 1011 cm−2 erg−1. The fraction accounts for the number of TMs used. The spectral model assumed here is a power law with an index Γ = 2 with absorption NH = 2 × 1020 cm−2. (6) Image count rate averaged after subtracting the instrumental background. (7) Estimated surface brightness after subtracting the instrumental background. (8) Estimated total flux of the western sky (180 < l < 360). The factors quoted here are based on the modeling assumptions and should be interpreted with caution due to the associated uncertainty. The errors quoted above are the statistical uncertainties.

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