The X-ray catalog of S82-XL is available for download (S82-XL_FINAL_XRAY.fits.zip). Information on each column is stored in the header file. If you use the catalog, please cite our paper Peca et al. 2024
This repository contains some of the n-dim array used in Peca et al. 2023 (see full paper for details):
- The
Corrections
folder contains the corrections to derive intrinsic AGN distributions. - The
XLF
folder contains the derived X-ray luminosity function. To usePeca23_XLF.py
you need to also downloadPeca23_XLF.npy
in the same folder. See below how to use the XLF and obtain the number density of AGN [Mpc-3] for a given luminosity and redshift bins or single values.
These files are free to use, but if you use them, please cite our paper at this link.
This script (Peca23_XLF.py) computes and plots the X-ray Luminosity Function (XLF) based on a provided dataset. It can evaluate the XLF at specific points or integrate over specified luminosity and redshift ranges.
To evaluate the XLF at a specific luminosity (Lx
) and redshift (z
):
python Peca23_XLF.py <log Lx> <z>
The result will be printed in the terminal.
To integrate the XLF over a range of luminosities (Lx_min to Lx_max) and redshifts (z_min to z_max):
python Peca23_XLF.py <log Lx_min> <log Lx_max> <z_min> <z_max>
The result will be printed in the terminal.
To integrate the XLF over a range of luminosities (Lx_min to Lx_max) and fixed redshift:
python Peca23_XLF.py <log Lx_min> <log Lx_max> <z>
NOTE: The script will print a warning if the provided values are outside the predefined ranges (log Lx [42-47], z [0,4]) derived in Peca et al. 2023. For larger ranges, the code will compute a linear extrapolation, so use it with caution.
NOTE: A very small number of C-thick AGN were discovered in Peca+23, therefore this XLF has to be considered reliable up to
The script will automatically print the 3D XLF with the requested volume density in red. To disallow the plotting option just add --plot=False