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IPTA DR2 - GWB analysis MCMC output

Authors: International Pulsar Timing Array Collaboration;

IPTA DR2 - GWB analysis MCMC output

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 provided in a README file. Each row of the chain file is one sample from the model posterior. The first samples at the beginning of the MCMC are the "burn-in" phase, before the chain has converged to the posterior. We recommend discarding the first ~25% of samples before using them to make inferences.

Keywords

pulsar timing array, gravitational waves

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    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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download
citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
views
OpenAIRE UsageCountsViews provided by UsageCounts
downloads
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Funded byView all
NSF| The NANOGrav Physics Frontiers Center
Project
  • Funder: National Science Foundation (NSF)
  • Project Code: 2020265
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Physics
,
NSF| Enabling multi-messenger science with pulsar timing arrays
Project
  • Funder: National Science Foundation (NSF)
  • Project Code: 1815664
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
result:project:semrel
,
EC| B Massive
Project
B Massive
Binary massive black hole astrophysics
  • Funder: European Commission (EC)
  • Project Code: 818691
  • Funding stream: H2020 | ERC | ERC-COG
result:project:semrel
,
NSERC
Project
  • Funder: Natural Sciences and Engineering Research Council of Canada (NSERC)
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