Table 1
[CII], [OI], and TIR surface brightnesses in defined apertures.
# | pos x | pos y | Angle | [CII] | [CII]unc | [OI] | [OI]unc | TIR | TIRunc |
[pix] | [pix] | [deg] | W/m2/sr | rel. | W/m2/sr | rel. | W/m2/sr | rel. | |
|
|||||||||
1 | 149 | 144 | 15 | – | – | – | – | 1.29e-4 | 0.09 |
2 | 146 | 143 | 29 | 1.12e-6 | 0.01 | 2.43e-7 | 0.12 | 2.64e-4 | 0.07 |
3 | 143 | 145 | 49 | 1.13e-6 | 0.01 | 3.33e-7 | 0.06 | 2.84e-4 | 0.04 |
4 | 141 | 148 | 68 | 1.62e-6 | 0.01 | 4.91e-7 | 0.04 | 4.54e-4 | 0.04 |
5 | 141 | 151 | 85 | 1.75e-6 | 0.01 | 5.40e-7 | 0.03 | 4.88e-4 | 0.03 |
6 | 142 | 154 | 102 | 1.60e-6 | 0.01 | 4.24e-7 | 0.05 | 3.98e-4 | 0.03 |
7 | 143 | 156 | 117 | 1.11e-6 | 0.01 | 2.72e-7 | 0.09 | 2.94e-4 | 0.03 |
8 | 145 | 158 | 135 | 8.87e-7 | 0.02 | 2.00e-7 | 0.23 | 2.56e-4 | 0.04 |
9 | 148 | 159 | 157 | – | – | – | – | 2.70e-4 | 0.03 |
10 | 151 | 159 | 180 | – | – | – | – | 2.56e-4 | 0.03 |
11 | 155 | 161 | 205 | 8.50e-7 | 0.02 | 1.31e-7 | 0.19 | 2.20e-4 | 0.03 |
12 | 157 | 161 | 213 | 7.83e-7 | 0.02 | 1.69e-7 | 0.11 | 2.12e-4 | 0.03 |
13 | 160 | 160 | 229 | 1.05e-6 | 0.01 | 2.94e-7 | 0.06 | 2.66e-4 | 0.03 |
14 | 161 | 157 | 243 | 1.34e-6 | 0.01 | 3.70e-7 | 0.05 | 3.28e-4 | 0.03 |
15 | 161 | 154 | 259 | 1.44e-6 | 0.01 | 3.82e-7 | 0.05 | 3.54e-4 | 0.03 |
16 | 161 | 151 | 275 | 1.40e-6 | 0.01 | 4.34e-7 | 0.08 | 3.38e-4 | 0.03 |
17 | 159 | 148 | 297 | – | – | – | – | 2.88e-4 | 0.05 |
18 | 156 | 146 | 320 | – | – | – | – | 3.42e-4 | 0.10 |
19 | 154 | 145 | 337 | – | – | – | – | 3.14e-4 | 0.12 |
20 | 152 | 144 | 353 | – | – | – | – | 2.56e-4 | 0.12 |
Notes. [CII] and [OI] emission line fluxes, TIR continuum flux, and their relative uncertainties in 3 × 3 pixel (12″ × 12″) apertures. Central positions (in TIR map pixels) of the apertures are given in the 2nd and 3rd columns. The order of the apertures (angles) here is clockwise (subsequently following the direction of gas motion), starting from due south. For reference, pixel (151, 152) corresponds to the galaxy center (RA 12h50m53.18s, Dec 41d07m12.0s).
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