matteolucchini1
matteolucchini1
Hi everyone, I'm having an issue with the modelling interface. I'm modelling the PSD of an X-ray binary trying to identify and subtract the QPOs from the broadband noise, and...
### Description of the Bug Per the title, the spectra loaded with the two different methods look slightly different. The script below uses the same obsid as the documentation, and...
### Description of the Bug We typically have two ways to construct arrays of Fourier frequency. One is to take the size of a segment to calculate the number of...
Currently the radiative term assumes we are always in the Thomson regime. It may be worth using the approach here https://ui.adsabs.harvard.edu/abs/2002ApJ...568L..81D/abstract to include a KN term (depending on the photon...
https://ui.adsabs.harvard.edu/abs/2006A%26A...451..739K/abstract have a slightly better treatment to handle the transition between the two regimes, compared to what we have now
Especially for the mixed class, this would help with avoiding having a large spike when transitioning from thermal to non-thermal particles for large values of f_nth.
Have methods for both BH scale units and cgs units
Per title, we can only do low redshift blazars right now
Ideally we would like the option of treating a hollow sheath, rather than a full cylinder. That requires changing the radiative calculations. For IC it's messy because of the RT...
Include pair annihilation/creation/gamma ray absorption, Wein spectra, Bremsstrahlung