relxill: Reflection models of black hole accretion disks
Abstract: relxill self-consistently connects an angle-dependent reflection model constructed with XILLVER (http://www.srl.caltech.edu/personnel/ja ... index.html) with the relativistic blurring code RELLINE (ascl:1505.021). It calculates the proper emission angle of the radiation at each point on the accretion disk and then takes the corresponding reflection spectrum into account.
Credit: Dauser, T.; García, J.; Parker, M. L.; Fabian, A. C.; Wilms, J.; Lohfink, A.; Kallman, T. R.; Steiner, J. F.; McClintock, J. E.; Brenneman, L.; Eikmann, W.; Reynolds, C. S.; Tombesi, F.
Site: https://github.com/thdauser/relxill
https://ui.adsabs.harvard.edu/abs/2016A%26A...590A..76D
Bibcode: 2020ascl.soft10015D
ID: ascl:2010.015