Pith Number

pith:EHYGW2Z5

pith:2025:EHYGW2Z5X2V7BPJS2HICSY3XT2

not attested not anchored not stored refs pending

Dark Energy Survey: Modeling strategy for multiprobe cluster cosmology and validation for the Full Six-year Dataset

A. A. Plazas Malag\'on, A. Carnero Rosell, A. Choi, A. Fert\'e, A. K. Romer, A. Palmese, A. Porredon, A. R. Walker, Chihway Chang, Chun-Hao To, D. Anbajagane, David H. Weinberg, D. Bacon, D. Brooks, D. Gruen, D. L. Hollowood, D. Sanchez Cid, Eduardo Rozo, E. Gaztanaga, Elisabeth Krause, E. Sanchez, E. Suchyta, F. Andrade-Oliveira, G. Giannini, G. Gutierrez, G. Tarle, Hao-Yi Wu, I. Sevilla-Noarbe, J. Blazek, J. Carretero, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garc\'ia-Bellido, J. J. Mohr, J. L. Marshall, J. Mena-Fern, J. Muir, J. Myles, J. Weller, K. Honscheid, K. Kuehn, L. N. da Costa, M. Aguena, M. Costanzi, M. E. S. Pereira, M. Gatti, M. R. Becker, M. Smith, N. Weaverdyck, P. Doel, Risa H. Wechsler, R. Miquel, S. Avila, S. Bocquet, S. Desai, S. Everett, S. Grandis, S. Lee, S. R. Hinton, S. Samuroff, T. Jeltema, T. M. C. Abbott, T. M. Davis, T. Shin, V. Vikram

arxiv:2503.13631 v1 · 2025-03-17 · astro-ph.CO · astro-ph.IM

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{EHYGW2Z5X2V7BPJS2HICSY3XT2}

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

4 papers in Pith

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

Challenges to the cosmological constant model following results from the Dark Energy Survey

Receipt and verification

First computed	2026-07-05T10:33:14.790370Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

21f06b6b3dbeabf0bd32d1d02963779e9d779ee6cb324e849e6da495e0ec2b88

Aliases

arxiv: 2503.13631 · arxiv_version: 2503.13631v1 · doi: 10.48550/arxiv.2503.13631 · pith_short_12: EHYGW2Z5X2V7 · pith_short_16: EHYGW2Z5X2V7BPJS · pith_short_8: EHYGW2Z5

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/EHYGW2Z5X2V7BPJS2HICSY3XT2 \
  | 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: 21f06b6b3dbeabf0bd32d1d02963779e9d779ee6cb324e849e6da495e0ec2b88

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "84f9544df60c5b7f7f3ea4b73cc946893f77d11a405289067dfb9eeef17a006e",
    "cross_cats_sorted": [
      "astro-ph.IM"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2025-03-17T18:28:14Z",
    "title_canon_sha256": "0f4516386dc4dd766cd65d3e1599c8e76de474d49a691b75f698fec0a83fb121"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2503.13631",
    "kind": "arxiv",
    "version": 1
  }
}