This scripts (jupyter notebook) in this github directory can be used to reproduce the main figures (the three figures with the rates) from the review paper by Mandel & Broekgaarden (2021) on "Rates of Compact Object Coalescence". In order to reproduce the figures one needs to download the data that is available on https://zenodo.org/record/7017532 doi:
To make the figures from the paper, put all the data (at least 26 files, unless you are only interested in reproducing one of the Compact Object flavors) in one directory and run the jupyter notebook in https://github.com/FloorBroekgaarden/Rates_of_Compact_Object_Coalescence/tree/main/plottingCode/Make_figures_Mandel_and_Broekgaarden_2021_COC_rates_review.ipynb
An example of one of the figures that the main code will repruduce is given below.
Variations of the figures that are available for use / to use in presentations can be found in the following two slide decks: (more are on the way)
Extra Vertical figures: https://github.com/FloorBroekgaarden/Rates_of_Compact_Object_Coalescence/tree/main/plottingCode/Extra_figures
If you use this data/code for publication, please cite both the paper: Mandel & Broekgaarden (2021) and the dataset on Zenodo through it's doi https://zenodo.org/record/7015954 doi:
an example bib is:
@MISC{ZenodoReview:2021, author = {Floor Broekgaarden and Ilya Mandel}, title = {{Data set from: Rates of Compact Object Coalescences}}, month = aug, year = 2022, note = {{Version 7 has fixed a few small typos from version 6, and has the flybys channel in a separate csv file and class version 6 includes the following changes: - Updated GWTC-3 BHBH, NSBH and NSNS rates with latest version population paper - Kinugawa et al. (2020) -> changed to Kinugawa et al. (2021) and updated the rates (we accidentaly quoted the wrong rates from the wrong paper) - Added Nuclear star cluster dynamics, with SMBH from Fragione et al. (2019) for BHBH, NSBH, and NSNS rates - Boekholt et al. (2022) added under AGN rates - added Stegmann (2022) to triple channels - added Olejek (2022) - Added Raveh et al. (2022) - added Zevin et al. (2022) - added Codazzo et al (2022) - added Michaely & Naoz (2022) - added Briel et al. (2022) - added Dorozsmai and Toonen (2022) Version 5 [used for published version of Living Reviews in relativity] has small changes in some of the label names, and has removed the Mandhai 2018 rates since these authors quote SGRB rates and not BNS rates. Version 4 has additional rates from recent papers and is updated to include the GWTC-3 results 11/19/21. This is the version that was used for the re-submitted paper. Version 3 has additional rates that we added after receiving useful feedback from the community (post ArXiv submission) Version 2 has updated and additional rates that we added. Version of the data that was used for the first ArXiv submission.}}, publisher = {Zenodo}, version = 7, doi = {10.5281/zenodo.7017532}, url = {https://doi.org/10.5281/zenodo.7017532} }
For any questions or inquiry, please email one of or both the authors: Ilya Mandel: ilya.mandel@monash.edu Floor Broekgaarden: floor.broekgaarden@cfa.harvard.edu
