Table A.1.
Pixel-by-pixel radio-FIR correlations for IC342.
| Region | Frequency | Component | Results | |||
|---|---|---|---|---|---|---|
| rp | Slope | t-value | n | |||
| IC 342 | OBS vs 70um | 0.87 ± 0.05 | 0.79 ± 0.03 | 4.19 | 184 | |
| 4.8 GHz | SYN vs 70um | 0.72 ± 0.06 | 0.73 ± 0.04 | 4.24 | 184 | |
| OBS vs 100um | 0.86 ± 0.04 | 0.75 ± 0.02 | 8.10 | 427 | ||
| SYN vs 100um | 0.75 ± 0.04 | 0.67 ± 0.06 | 7.92 | 379 | ||
| OBS vs 160um | 0.89 ± 0.03 | 0.69 ± 0.01 | 12.27 | 678 | ||
| SYN vs 160um | 0.74 ± 0.04 | 0.71 ± 0.02 | 11.66 | 395 | ||
| OBS vs 70um | 0.80 ± 0.05 | 0.70 ± 0.03 | 3.84 | 182 | ||
| 1.4 GHz | SYN vs 70um | 0.71 ± 0.05 | 0.67 ± 0.03 | 2.61 | 182 | |
| OBS vs 100um | 0.79 ± 0.03 | 0.58 ± 0.01 | 7.78 | 429 | ||
| SYN vs 100um | 0.71 ± 0.04 | 0.57 ± 0.02 | 7.64 | 384 | ||
| OBS vs 160um | 0.85 ± 0.04 | 0.48 ± 0.01 | 12.13 | 699 | ||
| SYN vs 160um | 0.72 ± 0.04 | 0.60 ± 0.02 | 11.57 | 403 | ||
| OBS vs 70um | 0.66 ± 0.06 | 0.74 ± 0.04 | 2.94 | 183 | ||
| 0.1 GHz | SYN vs 70um | 0.63 ± 0.06 | 0.68 ± 0.04 | 2.99 | 179 | |
| OBS vs 100um | 0.64 ± 0.04 | 0.73 ± 0.03 | 6.79 | 390 | ||
| SYN vs 100um | 0.62 ± 0.04 | 0.58 ± 0.02 | 6.65 | 358 | ||
| OBS vs 160um | 0.70 ± 0.04 | 0.70 ± 0.02 | 11.26 | 435 | ||
| SYN vs 160um | 0.64 ± 0.04 | 0.61 ± 0.02 | 10.94 | 373 | ||
| R1 | OBS vs 70um | 0.99 ± 0.03 | 0.86 ± 0.04 | 2.57 | 42 | |
| 4.8 GHz | SYN vs 70um | 0.96 ± 0.04 | 0.79 ± 0.08 | 2.61 | 42 | |
| OBS vs 100um | 0.99 ± 0.03 | 0.97 ± 0.06 | 3.41 | 42 | ||
| SYN vs 100um | 0.95 ± 0.04 | 0.88 ± 0.10 | 4.43 | 42 | ||
| OBS vs 160um | 0.97 ± 0.05 | 1.06 ± 0.08 | 4.45 | 42 | ||
| SYN vs 160um | 0.93 ± 0.05 | 0.97 ± 0.12 | 4.46 | 42 | ||
| OBS vs 70um | 0.99 ± 0.04 | 0.81 ± 0.06 | 2.51 | 42 | ||
| 1.4 GHz | SYN vs 70um | 0.98 ± 0.03 | 0.78 ± 0.07 | 2.61 | 42 | |
| OBS vs 100um | 0.98 ± 0.04 | 0.91 ± 0.07 | 3.37 | 42 | ||
| SYN vs 100um | 0.97 ± 0.03 | 0.87 ± 0.08 | 3.43 | 42 | ||
| OBS vs 160um | 0.96 ± 0.04 | 1.00 ± 0.08 | 4.43 | 42 | ||
| SYN vs 160um | 0.95 ± 0.04 | 0.95 ± 0.09 | 4.46 | 42 | ||
| OBS vs 70um | 0.94 ± 0.04 | 0.68 ± 0.06 | 2.36 | 42 | ||
| 0.1 GHz | SYN vs 70um | 0.88 ± 0.07 | 0.64 ± 0.07 | 2.60 | 42 | |
| OBS vs 100um | 0.95 ± 0.04 | 0.76 ± 0.06 | 3.42 | 42 | ||
| SYN vs 100um | 0.90 ± 0.06 | 0.71 ± 0.07 | 3.42 | 42 | ||
| OBS vs 160um | 0.96 ± 0.04 | 0.83 ± 0.07 | 4.40 | 42 | ||
| SYN vs 160um | 0.91 ± 0.06 | 0.78 ± 0.07 | 4.45 | 42 | ||
Notes. Pixel-by-pixel radio-FIR correlations for the observed radio continuum emission (OBS) and its synchrotron component (SYN) for the entire IC 342 and star-forming regions (R1). rp is the Pearson Correlation Coefficient, t-value the Student’s t-test, and n the number of independent data points.
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