Pith Number

pith:ZVY73PU6

pith:2015:ZVY73PU66RYD23HU3R73SNRYG5

not attested not anchored not stored refs pending

European Pulsar Timing Array Limits On An Isotropic Stochastic Gravitational-Wave Background

Alberto Sesana, Alberto Vecchio, Andrea Possenti, Antoine Lassus, Antoine Petiteau, Ben Stappers, Caterina Tiburzi, Cees G. Bassa, Chiara M. F. Mingarelli, David J. Champion, Delphine Perrodin, Gemma H. Janssen, Gilles Theureau, Gregory Desvignes, Ismael Cognard, Jason W. T. Hessels, Jonathan R. Gair, Joris P. W. Verbiest, K. J. Lee, Kuo Liu, Lindley Lentati, Lucas Guillemot, Mark B. Purver, Marta Burgay, Michael Kramer, Pablo A. Rosado, Patrick Brem, Patrick Lazarus, Ramesh Karuppusamy, R. Nicolas Caballero, Roy Smits, Rutger van Haasteren, Sotiris A. Sanidas, Stanislav Babak, Stefan Os{\l}owski, Stephen R. Taylor

arxiv:1504.03692 v3 · 2015-04-14 · astro-ph.CO · astro-ph.IM

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{ZVY73PU66RYD23HU3R73SNRYG5}

Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge

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

8 papers in Pith

New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions

Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition

TransitionListener v2.0 -- Robust gravitational wave predictions for cosmological phase transitions

Scalar induced gravitational waves review

Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter

Receipt and verification

First computed	2026-05-18T01:33:33.697342Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

cd71fdbe9ef4703d6cf4dc7fb93638377504306d0a1ed410b380bc056290770a

Aliases

arxiv: 1504.03692 · arxiv_version: 1504.03692v3 · doi: 10.48550/arxiv.1504.03692 · pith_short_12: ZVY73PU66RYD · pith_short_16: ZVY73PU66RYD23HU · pith_short_8: ZVY73PU6

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/ZVY73PU66RYD23HU3R73SNRYG5 \
  | 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: cd71fdbe9ef4703d6cf4dc7fb93638377504306d0a1ed410b380bc056290770a

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "ea6631741d1efda2ad5ebf92e3a0f22e4042de18cb231b305de9a339012a6b86",
    "cross_cats_sorted": [
      "astro-ph.IM"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2015-04-14T20:01:03Z",
    "title_canon_sha256": "778cee4f73f40ab4be5a0d70a423b133aab5ba0e051ef811088e5f8a6e672b9d"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1504.03692",
    "kind": "arxiv",
    "version": 3
  }
}