| | 10 | I've reprocessed the g-filter footprint data with the new dark (including the continuity correction), and it is currently stacking (label czw.footprint.dark,data_group = czw.20120308.footprint.g). The individual frames appear to have a smoother background, and this is reflected in an improved number of orphan detections. Directly comparing to the previous footprint reductions as before: |
| | 11 | |
| | 12 | [[Image(newdark_detections.png,400px)]] |
| | 13 | [[Image(relative_detections.png,400px)]] |
| | 14 | |
| | 15 | shows that the new dark model significantly decreases the number of singly detected objects. |