| Space Telescope Science Institute |
| COS Data Handbook 2.00 |
| help@stsci.edu |
The high voltage on the two FUV detector segments has been adjusted numerous times since launch in order to optimize the performance. Table B.1 lists the nominal high voltage values used since COS installation in 2009.The initial values used were identical to those used during ground testing. After early on-orbit tests showed that the gain of the MCPs was higher than expected on both segments, the voltages were lowered to return the gain to the prelaunch values. As described in Section 1.2.1, exposure to photon events lowered the gain in the spectral region at the original lifetime position, so the voltage was raised in March 2011 (Segment B) and March 2012 (Segment A) to keep the gain high enough to minimize throughput loss.