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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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