| | 1 | = This page discusses stacks with an excess in false detections in LAP.!ThreePi.20120706 = |
| | 2 | |
| | 3 | Bill Sweeney |
| | 4 | |
| | 5 | |
| | 6 | == False Detections from y band stacks 2012-12 == |
| | 7 | |
| | 8 | We have noticed that some skycells are getting large numbers of matched (forced photometry) detections. |
| | 9 | These are caused by false detections in the y band. Recall that forced photometry is performed for all y band sources |
| | 10 | that are not matched with a detection in another band while detections for the other filters must match 2 other bands |
| | 11 | before forced photometry is done. |
| | 12 | |
| | 13 | This plot shows the number of matched detetctions in i band verses the number of detected sources in y band. |
| | 14 | |
| | 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 | |