Gain Notes for Revolution 1457 This is one of the later revolutions in the mission where the calibration sources have become so weak that for the best energy determination and IC Gain History table is needed. NB!!!!! This is another revolution with a short period of switch off, after which there is a distinct settling period (gain rises significantly, but at different rates all over the microstrip plate). During these settling periods (i.e. the first few SCWs after switch on), the data should not be used for energy-sensitive purposes like spectra. OSA 10.0 will automatically ignore data from these periods. To get optimal results with this revolution it is necessary to use the IC gain history. See notes in revolutions prior to revolution 1433 to find out how to do this if you don't already know. Latest OSA software (version 10 and higher) automatically cuts out the first Science windows of data from each revolution to ensure that people do not use data from the instrument-settling period. This process can be overruled, but only by experienced users. JEM-X1: The Xe line analysis performed using the IC table shows very good gain correction with all science windows (taken 1 at a time) having a Xe level within about 2% of the ideal, except for the very first SCWs. As usual, it is recommended that users avoid the first few science windows for energy-sensitive applications (automatically removed by OSA 10.0). Calibration source number 4 (purple/orange) is no longer used for calibration purposes since an anode strip directly under the source has broken and no useable signal comes from this area of the detector any longer. CAO 29/9/2014 JEM-X2: The Xe line analysis performed using the IC table shows very good gain correction with all science windows (taken 1 at a time) having a Xe level well within 2% of the ideal, except for 4 SCWs during the two settling periods. So users should avoid the first few SCWs after both switch ons, for energy-sensitive applications (automatically removed by OSA 10.0). As with JEM-X1, source 4 is no longer used for energy correction purposes due to a broken anode strip CAO 15/10/2014