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Table B.1

Best-fit coefficients of the γ-ray model in each energy band and of the dust model.

γ-ray Energy band [MeV] E(BV)
model 102.6−102.8 102.8−103.2 103.2−103.6 103.6−105 102.6−105 model
qHI Cet 1.17 ± 0.06 1.10 ± 0.05 1.11 ± 0.05 1.02 ± 0.12 1.08 ± 0.03 1.61 ± 0.01
qHI TauS 1.22 ± 0.02 1.23 ± 0.02 1.17 ± 0.02 1.16 ± 0.04 1.20 ± 0.01 1.96 ± 0.01
qHI TauN 1.10 ± 0.02 1.04 ± 0.02 1.06 ± 0.02 1.13 ± 0.05 1.05 ± 0.01 1.70 ± 0.01
qHI TauM 1.26 ± 0.02 1.23 ± 0.02 1.19 ± 0.02 1.23 ± 0.04 1.23 ± 0.01 1.89 ± 0.03
qHI Cal 1.19 ± 0.05 1.18 ± 0.03 1.08 ± 0.04 1.15 ± 0.08 1.16 ± 0.02 2.11 ± 0.01
qHI Per 1.58 ± 0.14 1.32 ± 0.09 1.39 ± 0.11 1.08 ± 0.20 1.34 ± 0.06 2.55 ± 0.10
qHI Gal 0.57 ± 0.02 0.60 ± 0.02 0.57 ± 0.02 0.65 ± 0.04 0.57 ± 0.01 0.68 ± 0.06
qCO Cet 1.32 ± 0.71 2.51 ± 0.47 2.43 ± 0.51 0.00 ± 0.89 2.16 ± 0.30 4.64 ± 0.03
qCO TauS 1.91 ± 0.20 2.10 ± 0.15 2.08 ± 0.16 1.68 ± 0.30 2.01 ± 0.09 4.14 ± 0.02
qCO TauN 1.62 ± 0.10 1.62 ± 0.07 1.59 ± 0.08 1.67 ± 0.16 1.63 ± 0.05 4.16 ± 0.03
qCO TauM 1.81 ± 0.05 1.72 ± 0.04 1.64 ± 0.05 1.69 ± 0.09 1.68 ± 0.03 3.67 ± 0.03
qCO Cal 2.00 ± 0.10 1.92 ± 0.07 1.81 ± 0.08 1.81 ± 0.16 1.85 ± 0.05 3.92 ± 0.23
qCO Per 1.48 ± 0.12 1.63 ± 0.08 1.70 ± 0.09 1.97 ± 0.17 1.64 ± 0.05 2.52 ± 0.14
qCO Gal 1.98 ± 0.59 1.49 ± 0.39 2.09 ± 0.42 1.61 ± 0.74 1.58 ± 0.25 7.44 ± 0.02
qff 2.34 ± 0.69 3.14 ± 0.51 1.58 ± 0.55 3.27 ± 1.17 2.56 ± 0.32 2.09 ± 0.01
55.27 ± 3.40 60.38 ± 2.42 56.62 ± 2.66 61.48 ± 4.72 59.67 ± 1.53 2.92 ± 0.01
qDNM 45.82 ± 1.46 44.53 ± 1.06 43.23 ± 1.19 46.84 ± 2.38 45.03 ± 0.67 2.77 ± 0.01
qic 2.88 ± 0.77 4.54 ± 0.64 3.88 ± 0.65 2.48 ± 0.84 4.20 ± 0.36 -2.61 ± 0.01
qiso 1.39 ± 0.25 1.12 ± 0.28 0.70 ± 0.28 1.70 ± 0.27 1.07 ± 0.14

Notes. The q coefficients are expressed in 1020 cm−2 (K km s−1) for the CO; 3.8 × 1015 cm−2 Jy−1sr for the free-free; 1020 cm−2 mag−1 for the DNM and COsat; other q coefficients are simple normalization factors. The y coefficients are expressed as follows: (a) in 10−22 cm2; (b) in 10−2 mag K−1 km−1 s; (c) in 3.8 10−7 mag Jy−1 sr; (d) in 10−2 mag. The uncertainties reported are statistical only; the systematic uncertainties are 5% (based on the effective area uncertainties): https://fermi.gsfc.nasa.gov/ssc/data/analysis/LAT_caveats.html.

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