STScI Logo

Hubble Space Telescope

Post-Flash Summary

The ACS/WFC post-flash has been tested and a reference file has been created. The flash level is highly varied across both WFC CCDs, with a factor of two difference in signal level between the brightest part of the flash, and the darkest. The diagram below shows the level of flash across both CCDs. This image is in units of percentage, where 100% is the level of post-flash specified in APT and the ETC: 14 electrons/second. The image range is from 50 - 110 %, and the green portion of the image shows the area where the flash reaches 95-105 %. The pattern of the lamp is circular and slightly off-center of the chip gap between the two CCDs. The direction of the variation is such that the post-flash is brightest far from the readout amplifiers, where the CTE trailing is worse. Unfortunately, this variation in the post-flash leads to different levels of Poisson noise in different areas of the CCDs. The added noise from the post-flash, and the success of the pixel-based CTE correction already in place in CALACS results in a limited set of cases where post-flash may be helpful.


Post-flash is not recommended for most science observations. At present, post-flash is unnecessary in cases where the object is large or bright, as these objects are self-shielded from the worst effects of CTE trailing. Post-flash may be useful in cases of extremely faint unresolved/compact (less that ~10 pixels in size) targets imaged with short exposure times and/or narrow-band filters that would result in a background < 20e-. The ETC has now been modified to include a post-flash exposure, and will print an alert in the cases where post-flash is recommended. Unfortunately, the ETC does not account for CTE, so the user must manually adjust the brightness of their source in order to obtain the effective count rate. For point sources, this adjustment can be estimated using the equations from Chiaberge, M. in ACS ISR 2012-05 which have been incorporated into the ACS/WFC CTE Correction Calculator web tool. More information on CTE trailing in ACS and observation recommendations are documented in the CTE White Paper, and Ogaz, et al., 2013 (in prep). In future cycles, when CTE degradation will be even more severe, post-flash might become useful. The ACS Team will continue to monitor CTE degradation and the efficiency of post-flashing in mitigating CTE effects with a series of dedicated calibration programs. We encourage the users to periodically check the ACS website for updates.