Table 5
Radio-IR relations on pixel-by-pixel basis in N6946.
X | Y | b | rc | t | n |
|
|||||
RC(3.5) | I70 | 1.49 ± 0.04 | 0.90 ± 0.02 | 53.0 | 662 |
I100 | 1.49 ± 0.03 | 0.92 ± 0.01 | 61.8 | 696 | |
I160 | 1.20 ± 0.03 | 0.88 ± 0.01 | 55.0 | 883 | |
I250 | 1.03 ± 0.03 | 0.89 ± 0.02 | 56.3 | 834 | |
FF(3.5) | I70 | 0.92(0.95) ± 0.02 | 0.90(0.88) ± 0.02 | 52.5 | 650 |
I100 | 0.88(0.91) ± 0.02 | 0.90(0.89) ± 0.02 | 53.8 | 682 | |
I160 | 0.77(0.79) ± 0.01 | 0.88(0.88) ± 0.02 | 51.3 | 770 | |
I250 | 0.67(0.69) ± 0.01 | 0.87(0.86) ± 0.02 | 48.2 | 750 | |
SYN(3.5) | I70 | 1.60(1.58) ± 0.04 | 0.80(0.82) ± 0.02 | 33.8 | 644 |
I100 | 1.59(1.57) ± 0.04 | 0.84(0.84) ± 0.02 | 40.2 | 677 | |
I160 | 1.45(1.43) ± 0.03 | 0.86(0.87) ± 0.02 | 47.1 | 784 | |
I250 | 1.18(1.17) ± 0.03 | 0.86(0.87) ± 0.02 | 46.4 | 761 | |
|
|||||
RC(20) | I70 | 1.52 ± 0.03 | 0.87 ± 0.02 | 45.4 | 664 |
I100 | 1.48 ± 0.02 | 0.90 ± 0.02 | 54.4 | 697 | |
I160 | 1.16 ± 0.02 | 0.92 ± 0.01 | 70.1 | 911 | |
I250 | 1.02 ± 0.01 | 0.92 ± 0.01 | 68.3 | 850 | |
FF(20) | I70 | 0.92 ± 0.02 | 0.90 ± 0.02 | 50.3 | 656 |
I100 | 0.87 ± 0.02 | 0.90 ± 0.02 | 52.5 | 688 | |
I160 | 0.79 ± 0.01 | 0.88 ± 0.02 | 52.3 | 800 | |
I250 | 0.68 ± 0.01 | 0.87 ± 0.02 | 49.3 | 793 | |
SYN(20) | I70 | 1.53 ± 0.03 | 0.83 ± 0.02 | 38.2 | 661 |
I100 | 1.48 ± 0.03 | 0.87 ± 0.02 | 65.8 | 695 | |
I160 | 1.19 ± 0.02 | 0.91 ± 0.01 | 65.7 | 900 | |
I250 | 1.04 ± 0.02 | 0.90 ± 0.01 | 60.0 | 846 |
Notes.Pearson correlation coefficients rc and bisector slopes b, log (Y) ∝ blog (X), between the total RC, free-free (FF), synchrotron (SYN) from the TRT method and the far-infrared PACS and SPIRE bands. The values in parenthesis show the corresponding correlations when the observed Hα emission is directly used as the free-free tracer. Ordinary least-squares fits of bisector log (Y) ~ blog (X) are given through n pairs of (log X, log Y), where n is the number of independent points (Isobe et al. 1990); t is the Student’s t-test.
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