Trying to solve the differential Equations from Lipunova+99

Amoeba: an AGN Model of Optical Emissions Beyond steady-state Accretion disks

A tool for light curve extraction from the TESS FFIs.

A code to calculate the structure and spectrum of advection-dominated accretion flows (ADAFs)

A simple model of a thin alpha-accretion disc

1D disk models around black holes using DISKLAB code of Kees Dullemond and Til Birnstiel's

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 transfe…

This repository implements a python pipeline producing difference images of Pan-Starrs data.

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

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)

TESS FFI light curves fitted with effective PSF and decontaminated with Gaia DR2

Code for search of point-like sources of astrophysical neutrinos with 10-yr IceCube public data

A program which could generate highly realistic accretion disk around a Schwarzschild blackhole

Methods for determining the noise level of an unevenly sampled data set

Simple DAOPHOT-type photometry in Python translated from IDL AstroLib photometry algorithms. Please email me with bugs, suggestions, omissions, etc. The code is citable as part of the Astrophysics …

ZTF Uniform Depth Survey Image Processing Pipeline

Exploring the non-thermal radiation from pulsars at the center of our Galaxy!