Transient Detections and Other Real-Time Data Processing from MASTER-VWF Wide-Field Cameras
Figure 7
The number of identified stars as a function of magnitude. The straight lines indicate the and thresholds. Averaging was made within and bins in the right and left histograms, respectively. The right (coarser binned) histogram is smoother, resulting in reduced probability of accidentally reaching the threshold at a bright magnitude. It is therefore convenient to determine the limit on the coarsely binned histogram and then refine it on the finer-binned curve.
