Total far wing straylight, all scans.
|toward DC||from DC||toward DC||from DC||toward DC||from DC|
|396.5||2.8 (1.3e–13 M)||7.1 (4.6e–12 M)||2.4 (3.9e–13 M)||3.4 (3.3e–13 V)||2.4 (3.4e–13 M)||3.0 (4.1e–13 V)|
|436.4||4.3 (2.8e–14 L)||5.2 (2.1e–14 M)||2.9 (3.4e–13 M)||6.5 (6.3e–12 V)||3.4 (2.4e–13 M)||8.4 (5.4e–12 V)|
|538.0||1.5 (6.3e–13 V)||1.5 (9.1e–14 V)|
|557.6||1.8 (5.5e–13 M)||1.7 (8.3e–14 M)||0.7 (7.1e–13 M)||1.3 (3.9e–13 M)|
|630.2||1.3 (3.5e–13 M)||1.5 (6.8e–14 M)||0.7 (4.4e–13 M)||5 0.4 (4.1e–07 M)|
|854.2||1.3 (9.4e–13 L)||1.8 (1.7e–13 M)||1.1 (9.8e–13 L)||0.7 (8.4e–13 G)||1.0 (1.8e–12 M)||1.6 (1.0e–12 V)|
Notes. Each cell shows the best estimate straylight fraction in percent and in parentheses the outside-the-disk χ2 of the best fit and the initial of the kernel that gave the best fit. The reported straylight fraction is the median on-disk fraction, compare Fig. 11b. The DA “extra” data are from the 11:49 scans.
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