I need to keep track of what is totally necessary in the code for the imaging. I somewhat want to figure out if it's possible to produce time lags per disk patch - if so, this would be a really nice result for a paper, but definitely is very ambitious. I think that it would require considerable re-formatting to retain the imaging as well as the cross-spectrum. Currently, the code essentially makes the cross-spectrum for a single point source (which assumes all the signal is mixed up). Calculating the cross-spectrum per pixel might be quite difficult/pointless if the emission is mostly lagging the central accretion region (corona to disk + reflection processing).
I need to keep track of what is totally necessary in the code for the imaging. I somewhat want to figure out if it's possible to produce time lags per disk patch - if so, this would be a really nice result for a paper, but definitely is very ambitious. I think that it would require considerable re-formatting to retain the imaging as well as the cross-spectrum. Currently, the code essentially makes the cross-spectrum for a single point source (which assumes all the signal is mixed up). Calculating the cross-spectrum per pixel might be quite difficult/pointless if the emission is mostly lagging the central accretion region (corona to disk + reflection processing).