Pith Number

pith:JRAMGSZK

pith:2013:JRAMGSZKHGSQBYY3L3QBYRRU3D

not attested not anchored not stored refs pending

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples

Adam S. Bolton, Adrian M. Price-Whelan, Angela Burden, Antonio J. Cuesta, Ariel G. Sanchez, Ashley J. Ross, Benjamin A. Weaver, Beth Reid, Cameron K. McBride, Chia-Hsun Chuang, Christophe Yeche, Claudia G. Scoccola, Claudia Maraston, Cristiano G. Sabiu, Cullan Howlett, Daniel J. Eisenstein, Daniel Thomas, David A. Wake, David H. Weinberg, David J. Schlegel, David Kirkby, Donald P. Schneider, Eric Aubourg, Florian Beutler, Francesco Montesano, Francisco Prada, Gong-Bo Zhao, Hee-Jong Seo, Hong Guo, Idit Zehavi, James E. Gunn, J. Brinkmann, Jeremy L. Tinker, Joel R. Brownstein, John Parejko, Klaus Honscheid, Kyle S. Dawson, Lado Samushia, Lauren Anderson, Licia Verde, Marc Manera, Mariana Vargas Magana, Martin White, Matthew D. Olmstead, Michael A. Strauss, Michael Blanton, Molly E. C. Swanson, Natalie A. Roe, Nathalie Palanque-Delabrouille, Nicholas P. Ross, Nikhil Padmanabhan, Olga Mena, Patrick Petitjean, Ramin A. Skibba, Rita Tojeiro, Robert C. Nichol, Robert H. Lupton, Sebastian E. Nuza, Shirley Ho, Shun Saito, Stephanie Escoffier, Stephen Bailey, Vaishali Bhardwaj, Will J. Percival, Xiaoying Xu

arxiv:1312.4877 v2 · 2013-12-17 · astro-ph.CO

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{JRAMGSZKHGSQBYY3L3QBYRRU3D}

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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

10 papers in Pith

Cosmological constraints from neighbor-density-weighted marked correlation functions

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Barrow holographic dark energy interacting model in the presence of radiation and matter

DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions

Receipt and verification

First computed	2026-05-18T01:45:45.086437Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

4c40c34b2a39a500e31b5ee01c4634d8de4a0d491732073f430adb76f2911716

Aliases

arxiv: 1312.4877 · arxiv_version: 1312.4877v2 · doi: 10.48550/arxiv.1312.4877 · pith_short_12: JRAMGSZKHGSQ · pith_short_16: JRAMGSZKHGSQBYY3 · pith_short_8: JRAMGSZK

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/JRAMGSZKHGSQBYY3L3QBYRRU3D \
  | 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: 4c40c34b2a39a500e31b5ee01c4634d8de4a0d491732073f430adb76f2911716

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "9e98f8eb2da6495909b0a034bf5bcc98bc068b2a6e621fcba51cd5516c84472e",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2013-12-17T17:49:44Z",
    "title_canon_sha256": "a574458a6f83462ac2a142be7790df4a2cb3d813dc2d6aaf41d8cfdd4585e906"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1312.4877",
    "kind": "arxiv",
    "version": 2
  }
}