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Pith Number

pith:LKBAVKPL

pith:2023:LKBAVKPL7RRWSWDWNE36J7BXAG
not attested not anchored not stored refs pending

The second data release from the European Pulsar Timing Array II. Customised pulsar noise models for spatially correlated gravitational waves

A. Bathula, A. Berthereau, A. Chalumeau, A. Franchini, A. G. Lyne, A. Gopakumar, A. Jessner, A. K. Paladi, A. Parthasarathy, A. Petiteau, A. Possenti, A. Samajdar, A. S. Bak Nielsen, A. Sesana, A. Srivastava, A. Susobhanan, A. Vecchio, B. B. P. Perera, B. C. Joshi, B. Goncharov, B. W. Stappers, C. Dwivedi, C. G. Bassa, C. Tiburzi, D. Deb, D. Izquierdo-Villalba, D. J. Champion, D. Kharbanda, D. Perrodin, E. Bortolas, E. F. Keane, E. Graikou, E. van der Wateren, F. Iraci, F. Kareem, G. Desvignes, G. H. Janssen, G. Shaifullah, G. Theureau, H. Hu, H. Quelquejay Leclere, I. C. Ni\c{t}u, I. Cognard, J. Antoniadis, J. Jang, J. Jawor, J.-M. Grie{\ss}meier, J. P. W. Verbiest, J. R. Gair, J. Singha, J. Wang, J. W. McKee, K. J. Lee, K. Lackeos, K. Liu, K. Nobleson, K. Takahashi, L. Guillemot, L. Speri, L. Wang, M. A. Krishnakumar, M. Bagchi, M. B. Mickaliger, M. Bonetti, M. Burgay, M. Falxa, M. J. Keith, M. Kramer, M. Surnis, N. Dhanda-Batra, N. Kolhe, N. K. Porayko, P. Arumugam, P. Rana, P. R. Brook, P. Tarafdar, R. A. Main, R. D. Ferdman, R. Karuppusamy, R. N. Caballero, R. Spiewak, S. Arumugam, S. A. Sanidas, S. Babak, S. Chanlaridis, S. Chen, S. C. Susarla, S. Dandapat, S. Desai, S. Hisano, T. Kikunaga, T. Prabu, V. Venkatraman Krishnan, Y. Gupta, Y. J. Guo, Y. Liu, Y. Maan, Z. Wu

arxiv:2306.16225 v1 · 2023-06-28 · astro-ph.HE · astro-ph.IM

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Add to your LaTeX paper 
\usepackage{pith}
\pithnumber{LKBAVKPL7RRWSWDWNE36J7BXAG}

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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

6 papers in Pith

Inflationary interpretation of the gravitational-wave signal in the European Pulsar Timing Array DR2 with constraints
The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models
The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses
Thermodynamical uncertainties for primordial black holes from cosmological phase transitions
Detecting Chiral Gravitational Wave Background with a Dipole Pulsar Timing Array
Receipt and verification
First computed 2026-07-05T06:56:35.581921Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

5a820aa9ebfc636958766937e4fc3701a771243cce8c64f6b5e002fd9c31759e

Aliases

arxiv: 2306.16225 · arxiv_version: 2306.16225v1 · doi: 10.48550/arxiv.2306.16225 · pith_short_12: LKBAVKPL7RRW · pith_short_16: LKBAVKPL7RRWSWDW · pith_short_8: LKBAVKPL
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/LKBAVKPL7RRWSWDWNE36J7BXAG \
  | 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: 5a820aa9ebfc636958766937e4fc3701a771243cce8c64f6b5e002fd9c31759e
Canonical record JSON 
{
  "metadata": {
    "abstract_canon_sha256": "f7b5e2c61fdcde6ddab94105a6d9af0dc7af61373e6ea4bbd51d17fe67c1cc20",
    "cross_cats_sorted": [
      "astro-ph.IM"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.HE",
    "submitted_at": "2023-06-28T13:51:13Z",
    "title_canon_sha256": "2a99915f5a259628d39683a6ec715dfbac01fd4cda99b3feaa316f435ea75d12"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2306.16225",
    "kind": "arxiv",
    "version": 1
  }
}