| 15 | | [[BR]] |
| 16 | | [[Image(matched_i.jpg)]] |
| 17 | | |
| 18 | | If we plot the ratio of the number of matched detections to the number of detected sources for each band we can see these outliers. |
| 19 | | The following plots shows the ratio for the r band versus that in the ratio in i band for each stack. The plot on the left shows the full range |
| 20 | | including the outliers wile the plot on the right zooms in on the values near zero. |
| 21 | | [[Image(mdr.jpg)]] [[Image(mdrzoom.jpg)]] |
| 22 | | [[BR]] |
| 23 | | |
| 24 | | The plots for g and z show the same shape while the y band plot does not show the tail. |
| 25 | | |
| 26 | | [[Image(mdy.jpg)]] |
| 27 | | [[BR]] |
| 28 | | |
| 29 | | We propose re-running psphotStack for these skycells changing the rule that matched detections are created for all unmatched y band |
| 30 | | detections if some criteria is met. We can get rid of the worst of the outliers with the following cut. |
| 31 | | [[BR]] |
| 32 | | |
| 33 | | {{{ |
| 34 | | Nmatched_i / NDetected_i > 0.4 && Nmatched_r / NDetected_r > 0.6 |
| 35 | | }}} |
| 36 | | [[BR]] |
| 37 | | This effect is seen in 3% of the skycells north of 30 degrees declination. |
| 38 | | [[Image(mdr_cut.jpg)]] |
| 39 | | |
| 40 | | |
| 41 | | After testing a more conservative cut was chosen. It is based on the ratio of the number of sources in y |
| 42 | | to the number of sources detected in r, i, and z. |
| 43 | | |
| 44 | | Automatic forced photometry for sources detected in y band but not any other is disabled for skycells where |
| 45 | | |
| 46 | | {{{ |
| 47 | | (NDetected_y / NDetected_r) > 1.7 && (NDetected_y / NDetected_i > 1.6) && && (NDetectected_z > 1.65) |
| 48 | | }}} |
| 49 | | |
| 50 | | About 1 percent of skycells is affected by this feature. |
| 51 | | |
| | 16 | [[Image(y_detect.jpg)]] |