gabimoog

Astrophysicist working on black hole winds (or ultra fast outflows) in Active Galactic Nuclei

European Space AgencyUnited Kingdom

Pinned Repositories

BCES
Python module for performing linear regression for data with measurement errors and intrinsic scatter
Language:Jupyter Notebook10
corner.py
Make some beautiful corner plots
Language:Python0 1 00
multixstar
A python version of PVM XSTAR. Run XSTAR in parallel in as many cpu's as you want
Language:Python10
PyQSOFit
A code to fit the spectrum of quasar
Language:Jupyter Notebook0 1 00
python
This is the repository for Python, the radiative transfer code used to winds in AGN and other syatems
Language:C00
Python-Tutorials
Language:Jupyter Notebook0 1 00
qwind
A non-hydrodynamical model for AGN line-drive winds.
Language:Python00
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:Python00
uvwind
10
windy-blr-2020
Data and scripts for Matthews et al. 2020 paper entitled "Stratified disc wind models for the AGN broad-line region: ultraviolet, optical and X-ray properties"
Language:Ruby00

gabimoog/BCES
Python module for performing linear regression for data with measurement errors and intrinsic scatter
Language:Jupyter Notebook10
gabimoog/multixstar
A python version of PVM XSTAR. Run XSTAR in parallel in as many cpu's as you want
Language:Python10
gabimoog/uvwind
10
gabimoog/corner.py
Make some beautiful corner plots
Language:Python0 1 00
gabimoog/PyQSOFit
A code to fit the spectrum of quasar
Language:Jupyter Notebook0 1 00
gabimoog/python
This is the repository for Python, the radiative transfer code used to winds in AGN and other syatems
Language:C00
gabimoog/Python-Tutorials
Language:Jupyter Notebook0 1 00
gabimoog/qwind
A non-hydrodynamical model for AGN line-drive winds.
Language:Python00
gabimoog/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:Python00
gabimoog/windy-blr-2020
Data and scripts for Matthews et al. 2020 paper entitled "Stratified disc wind models for the AGN broad-line region: ultraviolet, optical and X-ray properties"
Language:Ruby00
gabimoog/xspec_emcee
Use EMCEE to do MCMC analyses of spectra in XSPEC
Language:Python1 0
gabimoog/xspec_emcee-1
Reimplementation of the MCMC algorithm emcee in XSPEC