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Pith Number

pith:3B5LXK2K

pith:2020:3B5LXK2KHHLUV3OSQ52TA2G737
not attested not anchored not stored refs pending

Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations

A. A. Plazas, A. Carnero Rosell, A. Choi, A. Drlica-Wagner, A. E. Evrard, A. Farahi, A. J. Ross, A. K. Romer, A. Palmese, A. Porredon, A. Roodman, B. Flaugher, B. Hoyle, B. Santiago, C. Chang, C. Conselice, C. Davis, C. S\'anchez, C. To, D. Brooks, D. Gruen, D. Huterer, D. J. James, D. L. Burke, D. L. Hollowood, D. L. Tucker, D. Thomas, E. Bertin, E. Gaztanaga, E. Krause, E. Rozo, E. Sanchez, E. Sheldon, E. S. Rykoff, E. Suchyta, F. Menanteau, F. Paz-Chinch\'on, G. Gutierrez, G. M. Bernstein, G. Tarle, H. T. Diehl, H. Wu, I. Ferrero, I. Sevilla-Noarbe, J. Annis, J. Blazek, J. Carretero, J. DeRose, J. Elvin-Poole, J. Frieman, J. Garc\'ia-Bellido, J. L. Marshall, J. Muir, J. Myles, J. P. Dietrich, J. Prat, J. Weller, J. Zuntz, K. Kuehn, L. N. da Costa, M. A. G. Maia, M. Aguena, M. A. Troxel, M. Carrasco Kind, M. Costanzi, M. Crocce, M. E. C. Swanson, M. E. S. Pereira, M. Gatti, M. Jarvis, M. Lima, M. M. Rau, M. R. Becker, M. Smith, N. Kuropatkin, N. MacCrann, O. Friedrich, P. Fosalba, P. Vielzeuf, R. A. Gruendl, R. Cawthon, R. H. Wechsler, R. Kron, R. Miquel, R. Morgan, S. Avila, S. Bhargava, S. Bocquet, S. Desai, S. Everett, S. L. Bridle, S. R. Hinton, S. Samuroff, S. Serrano, T. F. Eifler, T. Giannantonio, T. Jeltema, T. M. C. Abbott, T. McClintock, T. M. Davis, T. N. Varga, V. Miranda, V. Scarpine, W. G. Hartley, W. Wester (DES Collaboration), X. Fang, Y. Park, Y. Zhang

arxiv:2010.01138 v1 · 2020-10-02 · astro-ph.CO

Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3B5LXK2KHHLUV3OSQ52TA2G737}

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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

2 papers in Pith

Receipt and verification
First computed 2026-07-05T02:31:43.249485Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

d87abbab4a39d74aedd287753068dfdff61f11e7311903588c4510e1b97fa416

Aliases

arxiv: 2010.01138 · arxiv_version: 2010.01138v1 · doi: 10.48550/arxiv.2010.01138 · pith_short_12: 3B5LXK2KHHLU · pith_short_16: 3B5LXK2KHHLUV3OS · pith_short_8: 3B5LXK2K
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3B5LXK2KHHLUV3OSQ52TA2G737 \
  | 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: d87abbab4a39d74aedd287753068dfdff61f11e7311903588c4510e1b97fa416
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "af55915c5efb370dbb1f2d780719224a6e4fdd497940e12de31400f067ee6895",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2020-10-02T18:00:04Z",
    "title_canon_sha256": "59d55d4f6452459d5f8b7a2d986bb873e6a22a91c514dcf0d98e658e2b4c6a75"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2010.01138",
    "kind": "arxiv",
    "version": 1
  }
}