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The CTI and TGAIN corrections must also be applied when reprocessing the data.
For each year, level 2 event lists are created by reprocessing the data with the latest CIAO/CALDB version.
The TGAIN correction must also be applied when reprocessing the data; there is no CTI available for -110 °C.
The CXC is currently reprocessing the data from all observations obtained since the start of the mission.
By default, data obtained from the data archive and if using the default pix_adj values when reprocessing the data with chandra_repro has the EDSER sub-pixel event repositioning algorithm applied to ACIS data, and no pixel randomization is applied to HRC data.
Next, we examined whether the results could be improved by reprocessing the data from raw FASTQ sequence files.
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Once you have checked the V&V report for the observation, you should reprocess the data.
It is even possible to reprocess the data later to focus on a new subject of interest.
Users working with HRC-I data may wish run chandra_repro to reprocess the data and improve the gain calibration.
and then reprocess the data (e.g. with chandra_repro), to ensure that the latest calibration products have been used.
To reprocess the data (i.e. to apply new calibration), begin with the individual level 1 event files and process them separately.
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