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Table 2

Summary of simulation for photometric errors and completeness.

Flux Photometric errors Completenessa
(Jy) N2 N3 N4 S7 S9W S11 L15 L18W L24 MIR-S MIR-L
3.0e-06 ...b ... 0.817 ... ... ... ... ... ... 0.03 0.03
6.0e-06 ... 0.678 0.395 ... ... ... ... ... ... 0.04 0.03
1.2e-05 0.351 0.326 0.284 ... ... ... ... ... ... 0.10 0.04
2.4e-05 0.230 0.152 0.139 0.971 1.056 ... ... ... ... 0.34 0.06
4.7e-05 0.151 0.085 0.088 0.600 0.652 0.834 1.674 1.694 ... 0.70 0.19
9.4e-05 0.089 0.047 0.046 0.326 0.347 0.521 0.781 0.897 ... 0.85 0.54
1.9e-04 0.055 0.031 0.024 0.172 0.183 0.264 0.427 0.456 1.009 0.93 0.79
3.8e-04 0.027 0.015 0.011 0.087 0.094 0.143 0.244 0.261 0.504 0.95 0.89
7.5e-04 0.015 0.008 0.006 0.044 0.047 0.070 0.121 0.137 0.255 0.97 0.94
1.5e-03 0.007 0.004 0.003 0.022 0.024 0.034 0.066 0.069 0.134 0.99 0.95
3.0e-03 0.004 0.002 0.002 0.011 0.012 0.017 0.035 0.036 0.068 0.99 0.97
6.0e-03 0.002 0.001 0.001 0.006 0.007 0.009 0.018 0.017 0.035 0.99 0.98
1.2e-02 0.001 0.001 0.000 0.003 0.003 0.004 0.010 0.010 0.019 0.99 0.99
2.4e-02 0.001 0.000 0.000 0.002 0.002 0.002 0.005 0.005 0.010 0.99 0.99
4.7e-02 0.000 0.000 0.000 0.001 0.001 0.001 0.002 0.002 0.005 1.00 0.99
9.4e-02 0.000 0.000 0.000 0.001 0.000 0.001 0.001 0.002 0.003 1.00 1.00

Notes. 

(a)

Completeness in MIR-S and MIR-L detection images for the case of constant fluxes.

(b)

Photometric errors are given if |1 − Rave| < 0.2, where Rave is the average of the input-to-output flux ratio.

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