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Table 2

Best-fit γ-ray emissivities spectra per gas nucleon in the HI and DNM phases of the Reticulum and North Hydrus clouds.

Energy (MeV) qHI,Ret qDNM,Ret (1026 cm−2) qHI,HyiN qDNM,HyiN (1026 cm−2)
102.2–102.4 1.56 ± 0.23 ± 0.09 0.21 ± 1.22 ± 0.28 1.17 ± 0.15 ± 0.04 0.78 ± 0.52 ± 0.18
102.4–102.6 1.27 ± 0.13 ± 0.07 0.74 ± 0.61 ± 0.26 1.10 ± 0.08 ± 0.03 0.61 ± 0.26 ± 0.09
102.6–102.8 0.98 ± 0.10 ± 0.06 0.85 ± 0.41 ± 0.20 1.02 ± 0.06 ± 0.02 0.65 ± 0.17 ± 0.06
102.8–103.0 1.16 ± 0.08 ± 0.04 0.85 ± 0.29 ± 0.12 1.04 ± 0.04 ± 0.02 0.77 ± 0.12 ± 0.04
103.0–103.2 0.98 ± 0.07 ± 0.04 0.85 ± 0.27 ± 0.14 1.03 ± 0.04 ± 0.01 0.64 ± 0.11 ± 0.05
103.2–103.6 0.98 ± 0.07 ± 0.04 1.46 ± 0.26 ± 0.11 1.00 ± 0.04 ± 0.02 0.70 ± 0.11 ± 0.04
103.6–104.0 1.02 ± 0.16 ± 0.09 1.20 ± 0.55 ± 0.32 1.12 ± 0.09 ± 0.03 0.98 ± 0.23 ± 0.09
104.0–104.8 0.93 ± 0.38 ± 0.18 0.05 ± 1.14 ± 0.25 1.13 ± 0.21 ± 0.06 1.18 ± 0.55 ± 0.17
102.2–104.8 1.11 ± 0.04 ± 0.03 0.99 ± 0.15 ± 0.09 1.05 ± 0.02 ± 0.01 0.75 ± 0.07 ± 0.03

Notes. The first uncertainties are statistical (1σ) and the second give the standard deviations obtained in the jackknife fits.

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