Table 1
Best-fit parameters of the NIRCam versus NIRSpec pixel-by-pixel cross-calibration.
Filter | Overlapping IFU | Intercept A0,filter | Slope Afilter | Intrinsic scatter(a) σint | Pearson’s r |
---|---|---|---|---|---|
MJy sr−1 | MJy sr−1 | ||||
F187N | g235h-f170lp | −19 ± 1 | 0.994 ± 0.001 | 35 | 0.9955 |
F210M | g235h-f170lp | 5.3 ± 0.3 | 0.897 ± 0.003 | 7 | 0.9675 |
F212N | g235h-f170lp | 13.6 ± 0.5 | 0.80 ± 0.01 | −9.5 | 0.9094 |
Average (b) | g235h-f170lp | 0.980 ± 0.001 | |||
F323N | g395h-f2901p | 1.7 ± 0.3 | 0.919 ± 0.001 | 7 | 0.9973 |
F335M | g395h-f2901p | −1.9 ± 0.3 | 0.876 ± 0.001 | 10 | 0.9985 |
F405N | g395h-f2901p | 3 ± 1 | 0.901 ± 0.001 | 13 | 0.9986 |
F470N | g395h-f2901p | 9.6 ± 0.4 | 0.870 ± 0.001 | 13 | 0.9870 |
F480M | g395h-f2901p | 1.4 ± 0.3 | 0.861 ± 0.001 | 11 | 0.9929 |
Average (b) | g395h-f2901p | 0.8901 ± 0.0004 |
Notes. Statistical uncertainties in the slopes and intercepts are indicated. (a)Intrinsic scatter σint is defined as , where xi, yi are the individual measurements, σi is the uncertainty on yi, and f is the best-fit line. Negative σint indicates that the uncertainties are likely overestimated. (b)The uncertainty in the inverse-variance-weighted mean Afilter for each grating is the formal uncertainty. The true uncertainties on these factors are likely closer to the scatter in Afilter for filters within a given grating.
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