This week, I finished the last step of the cross-calibration analysis, which was finding cross-normalization
constants. To do that, I updated another XSPEC script that my mentor wrote, and I created a Python program
that would again write a new version of the script for each observatory pair. Each XSPEC program fits all the
data in a given pair simultaneously and records the flux from each instrument. I then calculated the
cross-normalization constant of each instrument pair by comparing the flux of one instrument to another.
The cross normalization constants for 2015 between NuSTAR and the other instruments.
Messed up contour plot showing how different the flux is between Swift and NuSTAR (from 2016).
Once I had finally found my cross-normalization constants, I began working on my final presentation. On Friday, I gave a short 5-minute presentation to the CRESST interns at NASA. Because I worked on fixing the Swift data for so long, I didn’t give myself enough time to prepare the presentation, and I kind of bombed it. Next week, I will be presenting again at a different event, so I’m hoping to do much better then!