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Scott Hagen (scotthgn)

scotthgn

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Scott Hagen's repositories

AGNvar

Python code for modelling spectral timing properties in AGN. Performs calculations of fully time-dependent SEDs following an input variable X-ray light-curve (See Hagen & Done (2023a)

Language:Jupyter NotebookLicense:MITStargazers:4Issues:2Issues:0

RELAGN

AGN SED model based off AGNSED (Kubota & Done 2018), but taking into account full GR ray tracing. These relativistic correction are calculated by doing the convolution with the relativistic transfer code KYCONV (Dovciak, Karas & Yaqoob 2004) at each radial annulus

Language:PythonLicense:MITStargazers:3Issues:2Issues:0

AGNvar2

Full Spectral Timing model for AGN. Calculates time-dependent SEDs, including an intrinsically variable disc (propagating fluctuations), disc reverberation, and wind re-processing

Language:PythonLicense:MITStargazers:1Issues:1Issues:0

AGNREF

Composite XSPEC model, consisting of a disc geometry as in AGNSED (Kubota & Done 2018) and an additional outflow component giving a thermal re-processor component and reflected component

Language:FortranLicense:MITStargazers:0Issues:0Issues:0

fAGNSED

Broad-band AGN SED model. Slight modification of AGNSED from Kubot & Done (2018), in that it now allows a colour-temperature correction on the standard outer disc region

Language:FortranLicense:MITStargazers:0Issues:1Issues:0