.....done: done: After all Detector Segment(s) have been illuminated with the spot, analyze the collected Raw Exposure(s). The Crosstalk Correction Matrix element (i, j) can be directly determined as the ratio of the flux measured in Segment j to the flux measured in Segment i, at the corresponding Pixel Coordinates. fin: Identify Pixel(s) affected by bright point Source(s), whose cross-talk affected counterparts contain nothing more than the AltPath: Data from background Basic Survey data or Compute the ratio of fluxes of those Pixel(s), per amp-amp pair Path Star Raster Scan step:9 Average the measurement over all data collected in a period of Exposures time shorter than the timescale of cross-talk changes on the Camera Produce Master Bias Exposure WBS: 02C.01.02.04 Create Master Bias Exposure from individual Bias Exposures Scenario Steps Summary Rejoins at Combine the Bias Exposure(s) to form the Master Bias Exposure Basic Path Store the Master Bias Exposure into the Calibration Database Produce Master Dark Exposure WBS: 02C.01.02.04 Create Master Dark Exposure from individual Dark Exposures Scenario Steps Summary Rejoins at Combine the Dark Exposure(s) to form the Master Dark Exposure Basic Path Store the Master Dark Exposure into the Calibration Database Produce Master Fringe Exposures WBS: 02C.01.02.04 For each Observing Filter, the Monochromatic Dome Flat Exposures will be used to construct the
.....done: done: After all Detector Segment(s) have been illuminated with the spot, analyze the collected Raw Exposure(s). The Crosstalk Correction Matrix element (i, j) can be directly determined as the ratio of the flux measured in Segment j to the flux measured in Segment i, at the corresponding Pixel Coordinates. fin: AltPath: Data from Survey data or Star Raster Scan Exposures Identify Pixel(s) affected by bright point Source(s), whose cross-talk affected counterparts contain nothing more than the background Compute the ratio of fluxes of those Pixel(s), per amp-amp pair Average the measurement over all data collected in a period of time shorter than the timescale of cross-talk changes on the Camera Basic Path step:9 Produce Master Bias Exposure WBS: 02C.01.02.04 Create Master Bias Exposure from individual Bias Exposures Scenario Steps Summary Rejoins at Basic Path Combine the Bias Exposure(s) to form the Master Bias Exposure Store the Master Bias Exposure into the Calibration Database Produce Master Dark Exposure WBS: 02C.01.02.04 Create Master Dark Exposure from individual Dark Exposures Scenario Steps Summary Rejoins at Basic Path Combine the Dark Exposure(s) to form the Master Dark Exposure Store the Master Dark Exposure into the Calibration Database Produce Master Fringe Exposures WBS: 02C.01.02.04 For each Observing Filter, the Monochromatic Dome Flat Exposures will be used to construct the