Pith Number

pith:KYT4JKMD

pith:2020:KYT4JKMDOLLJURDMTYRHATAYZW

not attested not anchored not stored refs pending

The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave Background

Adam Brazier, A. Miguel Holgado, Andrew R. Kaiser, Bence Becsy, Brent J. Shapiro-Albert, Caitlin A. Witt (for the NANOGrav Collaboration), Cherry Ng, Chiara M. F. Mingarelli, Daniel R. Stinebring, David J. Nice, David L. Kaplan, Deborah C. Good, Duncan R. Lorimer, Dustin R. Madison, Elizabeth C. Ferrara, Emmanuel Fonseca, Fronefield Crawford, Harsha Blumer, H. Thankful Cromartie, Ingrid H. Stairs, Jacob E. Turner, James M. Cordes, Jeffrey S. Hazboun, Jerry P. Sun, Jing Luo, Joey Shapiro Key, Joseph K. Swiggum, Joseph Simon, Justin A. Ellis, Kevin Stovall, Kristina Islo, Luke Zoltan Kelley, Maura A. McLaughlin, Megan E. DeCesar, Megan L. Jones, Michael T. Lam, Michele Vallisneri, Nathan Garver-Daniels, Neil J. Cornish, Nihan S. Pol, Nima Laal, Paul B. Demorest, Paul R. Brook, Paul S. Ray, Paul T. Baker, Peter A. Gentile, Renee Spiewak, Ross J. Jennings, Ryan S. Lynch, Sarah Burke-Spolaor, Sarah J. Vigeland, Scott M. Ransom, Shami Chatterjee, Siyuan Chen, Stephen R. Taylor, Timothy Dolch, Timothy T. Pennucci, T. Joseph W. Lazio, William Fiore, Xavier Siemens, Zaven Arzoumanian

arxiv:2009.04496 v2 · 2020-09-09 · astro-ph.HE · astro-ph.GA · gr-qc

Open paper page JSON Open Graph Bundle Merged state Verified badge What is a Pith Number?

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{KYT4JKMDOLLJURDMTYRHATAYZW}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Cited by

15 papers in Pith

A Joint Optimal Search for Gravitational Waves from Resolved and Unresolved Supermassive Binary Black Holes with Pulsar Timing Arrays

Inflationary interpretation of the gravitational-wave signal in the European Pulsar Timing Array DR2 with constraints

PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference

Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks

Whispers of Supergravity in Gravitational Wave Backgrounds: Determining the Gravitino Mass from Cosmic Thermal History

Receipt and verification

First computed	2026-07-05T02:05:27.984953Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

5627c4a98372d69a446c9e22704c18cd9e0dadebe28f1c68c12bae4c2b89857a

Aliases

arxiv: 2009.04496 · arxiv_version: 2009.04496v2 · doi: 10.48550/arxiv.2009.04496 · pith_short_12: KYT4JKMDOLLJ · pith_short_16: KYT4JKMDOLLJURDM · pith_short_8: KYT4JKMD

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/KYT4JKMDOLLJURDMTYRHATAYZW \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 5627c4a98372d69a446c9e22704c18cd9e0dadebe28f1c68c12bae4c2b89857a

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "2a4f101773b8d85da7c6a12dcfc457b3ae0bd452d10289edc20dfdc0818594be",
    "cross_cats_sorted": [
      "astro-ph.GA",
      "gr-qc"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2020-09-09T18:09:01Z",
    "title_canon_sha256": "b7e2ebdc4414b449dde9cc4660cd3fb64bb5ab547d56dd375c473c9041a83904"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2009.04496",
    "kind": "arxiv",
    "version": 2
  }
}