ASCL Code Record
[ascl:2010.015]
relxill: Reflection models of black hole accretion disks
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.
relxill self-consistently connects an angle-dependent reflection model constructed with XILLVER (http://www.srl.caltech.edu/personnel/javier/xillver/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.
- Code site:
- http://www.sternwarte.uni-erlangen.de/~dauser/research/relxill/index.html https://github.com/thdauser/relxill
- Described in:
- https://ui.adsabs.harvard.edu/abs/2014ApJ...782...76G https://ui.adsabs.harvard.edu/abs/2014MNRAS.444L.100D https://ui.adsabs.harvard.edu/abs/2016A%26A...590A..76D https://ui.adsabs.harvard.edu/abs/2022MNRAS.514.3965D%2F
- Bibcode:
- 2020ascl.soft10015D
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