Best-fitting normalization values for the three X-ray sky background model components.
| Local Hot Bubble . | Galactic halo . | Cosmic X-ray background . |
|---|---|---|
| (cm|$^{-5}$| arcmin|$^{-2}$|) . | (cm|$^{-5}$| arcmin|$^{-2}$|) . | (photons keV|$^{-1}$| cm|$^{-2}$| s|$^{-1}$| arcmin|$^{-2}$|) . |
| (4.9 |$\pm$| |$0.1)\times 10^{-7}$| | (1.04 |$\pm$| |$0.06)\times 10^{-6}$| | (9.5 |$\pm$| |$0.9)\times 10^{-7}$| |
| Local Hot Bubble . | Galactic halo . | Cosmic X-ray background . |
|---|---|---|
| (cm|$^{-5}$| arcmin|$^{-2}$|) . | (cm|$^{-5}$| arcmin|$^{-2}$|) . | (photons keV|$^{-1}$| cm|$^{-2}$| s|$^{-1}$| arcmin|$^{-2}$|) . |
| (4.9 |$\pm$| |$0.1)\times 10^{-7}$| | (1.04 |$\pm$| |$0.06)\times 10^{-6}$| | (9.5 |$\pm$| |$0.9)\times 10^{-7}$| |
Best-fitting normalization values for the three X-ray sky background model components.
| Local Hot Bubble . | Galactic halo . | Cosmic X-ray background . |
|---|---|---|
| (cm|$^{-5}$| arcmin|$^{-2}$|) . | (cm|$^{-5}$| arcmin|$^{-2}$|) . | (photons keV|$^{-1}$| cm|$^{-2}$| s|$^{-1}$| arcmin|$^{-2}$|) . |
| (4.9 |$\pm$| |$0.1)\times 10^{-7}$| | (1.04 |$\pm$| |$0.06)\times 10^{-6}$| | (9.5 |$\pm$| |$0.9)\times 10^{-7}$| |
| Local Hot Bubble . | Galactic halo . | Cosmic X-ray background . |
|---|---|---|
| (cm|$^{-5}$| arcmin|$^{-2}$|) . | (cm|$^{-5}$| arcmin|$^{-2}$|) . | (photons keV|$^{-1}$| cm|$^{-2}$| s|$^{-1}$| arcmin|$^{-2}$|) . |
| (4.9 |$\pm$| |$0.1)\times 10^{-7}$| | (1.04 |$\pm$| |$0.06)\times 10^{-6}$| | (9.5 |$\pm$| |$0.9)\times 10^{-7}$| |
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