Pith Number

pith:WM7O6EZY

pith:2014:WM7O6EZYKOWHCEINFOC5DBOFRF

not attested not anchored not stored refs pending

Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

A. Conley, A. Goobar, A. G. Riess, A. M. Mour\~ao, A. M\"oller, A. V. Filippenko, B. A. Bassett, C. Balland, C. B. D'Andrea, C. J. Hogan, C. J. Pritchet, C. J. Wheeler, C. Lidman, D. A. Howell, D. Cinabro, D. Fouchez, D. Hardin, D. L. DePoy, D. P. Schneider, F. Cellier-Holzem, G. J. Hill, G. Leloudas, H. Campbell, I. M. Hook, J. A. Frieman, J. Guy, J. L. Marshall, J. L. Prieto, J. Marriner, J. Mosher, J. Neveu, J. Sollerman, K. Schahmaneche, L. Galbany, L. Le Guillou, M. Betoule, M. Doi, M. D. Olmstead, M. Konig, M. Richmond, M. Sako, M. Smith, M. Sullivan, N. A. Walton, N. Palanque-Delabrouille, N. Regnault, P. Astier, P. El-Hage, P. J. Brown, R. Biswas, R. G. Carlberg, R. Hlozek, R. J. Foley, R. Kessler, R. Nichol, R. Pain, R. R. Gupta, R. S. Ellis, S. Fabbro, S. Kuhlmann, S. Perlmutter, S. W. Jha, V. Ruhlmann-Kleider

arxiv:1401.4064 v2 · 2014-01-16 · astro-ph.CO

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{WM7O6EZYKOWHCEINFOC5DBOFRF}

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

18 papers in Pith

Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference

DESI DR2 Reference Mocks: Clustering results from UCHUU ELGs and QSOs

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension

Mapping the Universe as a Bianchi I cosmology with Gaia data

Testing cosmic anisotropy with the Combo correlation of gamma-ray bursts

Receipt and verification

First computed	2026-05-18T01:45:24.807730Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

b33eef133853ac71110d2b85d185c5896cb1ae2e4b5c98513cae7a04fee3bc0c

Aliases

arxiv: 1401.4064 · arxiv_version: 1401.4064v2 · doi: 10.48550/arxiv.1401.4064 · pith_short_12: WM7O6EZYKOWH · pith_short_16: WM7O6EZYKOWHCEIN · pith_short_8: WM7O6EZY

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/WM7O6EZYKOWHCEINFOC5DBOFRF \
  | 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: b33eef133853ac71110d2b85d185c5896cb1ae2e4b5c98513cae7a04fee3bc0c

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "6736ab470355c2f5396ee0ea2f50f5080ea694056c7243a587235a6aaabeedcc",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2014-01-16T15:30:53Z",
    "title_canon_sha256": "f72322ea91a2c6554a9756a8928c8e56b26945531b102903adaf6de713a6ee25"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1401.4064",
    "kind": "arxiv",
    "version": 2
  }
}