KDE Representations of the Gravitational Wave Background Free Spectra Present in the NANOGrav 15-Year Dataset
Authors/Creators
Contributors
Data curator:
Project leader (2):
Project manager:
- 1. Vanderbilt University
- 2. University of Wisconsin–Milwaukee
- 3. West Virginia University
Description
OVERVIEW
----------------
This is a downloadable file of probability densities from KDEs (Kernel Density Estimator) of free spectrum analyses of the NANOGrav 15yr Dataset (DOI 10.5281/zenodo.7967584) that can be used with the Ceffyl and PTArcade packages. Please see the GitHub page for Ceffyl/PTArcade installation details and usage information.
Details on how this data product was produced can be found in Lamb, Taylor & van Haasteren 2023 (DOI 10.1103/PhysRevD.108.103019).
DIRECTORY AND FILE STRUCTURE
----------------------------------------------------
Each directory contains a file with log-pdfs representing their corresponding free spectra (`density.npy`), the frequencies at which they were analysed (`freqs.npy`), the grid-points at which each log-pdf was computed (`log10rhogrid.npy`), frequency labels (`log10rholabels.txt`), analysis label (`pulsar_list.txt`), an array of bandwidths computed using the Sheather-Jones method (see Lamb et al. 2023; 'bandwidths.npy'), and a file with some metadata about the data (`log.txt`).
./30f_fs{cp}_ceffyl
- A representation of a 30 frequency CURN free spectrum.
./30f_fs{hd}_ceffyl
- A representation of a 30 frequency HD-correlated free spectrum
./30f_fs{hd+mp+dp+cp}_ceffyl_hd-only
- A representation of an analysis that simultaneously modeled a HD-correlated free spectrum, a MP-correlated free spectrum, a DP-correlated free spectrum, and a CURN free spectrum. Only the HD component is represented here.
./README
- this is a readme
SOFTWARE
------------------
This data should ideally be used with the latest versions of:
- ceffyl (https://github.com/astrolamb/ceffyl)
- PTArcade (https://github.com/andrea-mitridate/PTArcade)
PLANNED REVISIONS
---------------------------------
None
CHANGE LOG
----------------------
07/08/2026 - Corrected data set after finding a bug in our sampler
- A bug was found in the parallel tempering sub-routine of `PTMCMCSampler`, an MCMC sampler that was used to estimate the free spectrum posteriors of the NANOGrav 15yr data set. This release corrects the posteriors which were biased by this bug.
- Details of the bug can be found here: Pull Release 58
- This bug affected population inference of SMBHBs. See the following erratum: Agazie et al 2026 ApJL1006 L67
- We re-ran every free spectrum with the exception of `30f_fs{hd+mp+dp}_ceffyl_hd-only` and `30f_fs{hd}_100fDMGP_ceffyl`
10/12/2023 - updated KDE representations
A bug was found that produced a poor reflection at the lower prior boundary. Hence, data was being represented well at the lower prior boundary. This has now been corrected.
Notes
Files
ceffyl_data.zip
Additional details
Related works
- Is documented by
- Journal article: 10.3847/2041-8213/ae8764 (DOI)
- Is new version of
- Dataset: 10.5281/zenodo.10344086 (DOI)
- Is supplement to
- Journal article: 10.3847/2041-8213/acdac6 (DOI)
- References
- Journal article: 10.1103/PhysRevD.108.103019 (DOI)
Funding
- U.S. National Science Foundation
- The NANOGrav Physics Frontiers Center 2020265
- U.S. National Science Foundation
- NANOGrav Physics Frontier Center 1430284
References
- Gabriella Agazie et al 2023 ApJL 951 L8 (DOI 10.3847/2041-8213/acdac6)
- Lamb, Taylor & van Haasteren 2023 Phys. Rev. D 108, 103019 (DOI 10.1103/PhysRevD.108.103019)
- Agazie et al 2026 ApJL 1006 L67 (10.3847/2041-8213/ae8764)