Homogenized AGN catalogue and luminosity function analysis code from Kulkarni et al. 2018.
This repository contains three things:
- A homogeneous catalogue of 83,488 AGN between redshift 0 and 7.5, with rest-frame UV magnitudes, redshifts, and selection probabilities.
- Code to derive luminosity functions from this data
- Code to model hydrogen and helium reionization
The commit tagged
v3.0 reproduces the results from Kulkarni et al. 2018.
Data_new subdirectory contains the AGN catalogue in ASCII text files. Comments in the files explain their structure. See Section 2 of the paper for details on the original references for these data and how we homogenise them. Use
data.py to visualise the full catalogue in the style of Figure 1 of the paper. Luminosity functions in bins of redshift and magnitude are implemented in
drawlf.py. These are shown as points in, e.g., Figure 3 of the paper. Detailed definitions are in Section 3.1 of the paper.Double-power-law luminosity function models are derived in the
lf class, defined in
bins.py for examples on how to use this class. The latter is used by
mosaic.py to produce Figure 3 of the paper. Details of this modelling is in Section 3.2 of the paper. Global models of luminosity function evolution are implemented in
lfg_multiple.py for examples of how to use these. Three such models are discussed in Section 3.3 of the paper. Hydrogen-ionizing emissivity is modelled in
gammapi.py. The hydrogen-photoionization rate is modelled in
rtg2.py. Code in
qhe.py models Helium reionization. The methods behind these codes is discussed in Section 4 of the paper.
1. Where do I start?
Begin by running lfi.py to get the luminosity function in a redshift bin.
2. How do I get the number density of AGN at a certain redshift?
Pass luminosity function models (instances of
composite.lf) to one of the functions in
3. I just want to know the value of one of the double-power-law parameters at a redshift
Pass an instance of
Girish Kulkarni (firstname.lastname@example.org)