research data . Dataset . 2022

IPTA DR2 - GWB analysis MCMC output

International Pulsar Timing Array Collaboration;
Open Access
  • Published: 12 Jan 2022
  • Publisher: Zenodo
Abstract
IPTA DR2 common red noise, MCMC output These files are the primary output from a Markov chain Monte Carlo (MCMC) sampling process. They are samples from the posterior probability distribution for a particular model described in the companion paper. Each zipped tarball contains four files. The "chain" file has several tab-separated columns, each of which corresponds to a model parameter, except the last four which are metadata. The parameter names (including metadata) are listed in the companion "params" file. The frequencies used in the common red noise models are listed in the "crn_frequencies" file. Additional information is...
Subjects
free text keywords: gravitational waves, pulsar timing array
Communities
Communities with gateway
OpenAIRE Connect image
Funded by
ANR| PTA-France
Project
PTA-France
Gravitational wave search with a Pulsar Timing Array in France
  • Funder: French National Research Agency (ANR) (ANR)
  • Project Code: ANR-18-CE31-0015
,
ARC| Discovery Early Career Researcher Award - Grant ID: DE210101738
Project
  • Funder: Australian Research Council (ARC) (ARC)
  • Project Code: DE210101738
  • Funding stream: Discovery Early Career Researcher Award
,
EC| B Massive
Project
B Massive
Binary massive black hole astrophysics
  • Funder: European Commission (EC)
  • Project Code: 818691
  • Funding stream: H2020 | ERC | ERC-COG
,
NSERC
Project
  • Funder: Natural Sciences and Engineering Research Council of Canada (NSERC)
Download fromView all 2 versions
Open Access
ZENODO
Dataset . 2022
Provider: ZENODO
Open Access
ZENODO
Dataset . 2022
Provider: Datacite
Any information missing or wrong?Report an Issue