Table 4.
H i Emissivity Scaling Factors
| Region | Complex | Scaling Factor |
Stata | Sys (Model)b |
Sys (Jackknife)c |
|---|---|---|---|---|---|
| A | Local | 0.99 | 0.02 |
+0.04 −0.14 |
0.08 |
| Low-Latitude IV Arch | 0.94 | 0.15 |
+0.26 −0.01 |
0.08 | |
| Complex A | <0.21 | <0.22 | <0.001 | ||
| B | Local | 0.94 | 0.07 |
+0.13 −0.22 |
0.08 |
| Lower IV Arch | 1.08 | 0.04 |
+0.10 −0.08 |
0.09 | |
| Upper IV Arch | <0.23 | <0.45 | <0.01 | ||
| C | Local | 1.08 | 0.04 |
+0.05 −0.09 |
0.09 |
| IV Spur | 0.68 | 0.06 |
+0.09 −0.03 |
0.06 | |
Notes. Upper limits are provided at 95% confidence level.
a
1σ statistical uncertainty from the likelihood analysis.
b
Systematic spread from varying some inputs to the γ-ray interstellar emission model (see Section 5.4.1).
c
1σ uncertainty or 95% c.l. upper limit from the distributions obtained with the jackknife test (see Section 5.4.2).