Pith Number

pith:EZCEEJIP

pith:2025:EZCEEJIPHW7MSAG7A54SKY4NZW

not attested not anchored not stored refs pending

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

A. Alarcon, A. A. Plazas Malag\'on, A. Carnero Rosell, A. Choi, A. Farahi, A. Fert\'e, A. K. Romer, A. Palmese, A. Porredon, A. Roodman, A. R. Walker, B. Flaugher, B. Yanny, C. Chang, C. Conselice, Chun-Hao To, C. Lidman, C. Zhou, D. Anbajagane, David H. Weinberg, D. Bacon, D. Brooks, DES Collaboration: T. M. C. Abbott, D. Gruen, D. L. Hollowood, D. Sanchez Cid, D. Thomas, E. Krause, E. Rozo, E. Sanchez, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. J. Castander, G. Giannini, G. Gutierrez, G. Tarle, H. Lin, H. T. Diehl, H.-Y. Wu, I. Harrison, I. Sevilla-Noarbe, J. Blazek, J. Carretero, J. Elvin-Poole, J. Esteves, J. Garc\'ia-Bellido, J. J. Mohr, J. L. Marshall, J. McCullough, J. Mena-Fern, J. Muir, J. Myles, J. Prat, J. Weller, K. Honscheid, L. N. da Costa, M. Aguena, M. A. Troxel, M. Costanzi, M. Crocce, M. E. S. Pereira, M. Gatti, M. Lima, M. Paterno, M. R. Becker, M. Smith, M. Yamamoto, N. Jeffrey, N. Weaverdyck, O. Lahav, P. Doel, P. Giles, R. A. Gruendl, R. H. Wechsler, R. L. C. Ogando, R. Miquel, S. Avila, S. Bhargava, S. Bocquet, S. Desai, S. Dodelson, S. Everett, S. Grandis, S. Lee, S. R. Hinton, T. Jeltema, T. M. Davis, V. Vikram, Y. Zhang

arxiv:2503.13632 v1 · 2025-03-17 · astro-ph.CO

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{EZCEEJIPHW7MSAG7A54SKY4NZW}

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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

5 papers in Pith

Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference

Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey

Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters

Photometric Redshift PDFs via Neural Network Classification for DESI Legacy Imaging Surveys and Pan-STARRS

Forward analytical model for the optical selection bias on galaxy cluster lensing profiles

Receipt and verification

First computed	2026-07-05T10:33:15.231677Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

264442250f3dbec900df077925638dcdbd25b8c4ccc5c726ce534e6d746cb81e

Aliases

arxiv: 2503.13632 · arxiv_version: 2503.13632v1 · doi: 10.48550/arxiv.2503.13632 · pith_short_12: EZCEEJIPHW7M · pith_short_16: EZCEEJIPHW7MSAG7 · pith_short_8: EZCEEJIP

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/EZCEEJIPHW7MSAG7A54SKY4NZW \
  | 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: 264442250f3dbec900df077925638dcdbd25b8c4ccc5c726ce534e6d746cb81e

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "754b3397976b9233e65855f0a1046791c691324ae8b7bccd9c39eb1e4a80b2e4",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2025-03-17T18:28:21Z",
    "title_canon_sha256": "f18e452f54e2eb4f53cdf84b1f357dd66087757e861f355fb2ab57b798ba8568"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2503.13632",
    "kind": "arxiv",
    "version": 1
  }
}