Pith Number

pith:QK4KAIWB

pith:2025:QK4KAIWBYIQWKQ3GTAXE4V7V73

not attested not anchored not stored refs pending

Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data

A. Aviles, A. Carnero Rosell, A. Cuceu, A. de la Macorra, A. de Mattia, A. Font-Ribera, A. J. Ross, A. Kremin, A. Leauthaud, A. Meisner, A. Mu\~noz-Guti\'errez, Arjun Dey, A. Shafieloo, B. A. Weaver, Biprateep Dey, C. Garcia-Quintero, C. Hahn, C. Howlett, C. Lamman, C. Ravoux, C. Y\`eche, C. Zhao, D. Bianchi, D. Brooks, D. Chebat, D. Huterer, D. Kirkby, D. Schlegel, D. Sprayberry, E. Burtin, E. Chaussidon, E. Gazta\~naga, E. Paillas, E. Sanchez, F. J. Castander, F. Prada, G. Gutierrez, G. Niz, G. Rossi, G. Tarl\'e, H. E. Noriega, H. Gil-Mar\'in, H. K. Herrera-Alcantar, H. Seo, I. P\'erez-R\`afols, J. Aguilar, J. A. Newman, J. Della Costa, J. E. Forero-Romero, J. Guy, J. Mena-Fern\'andez, J. Moustakas, J. Pan, J. Rohlf, J. Silber, K. Honscheid, K. Lodha, L. Le Guillou, M. E. Levi, M. Ishak, M. Landriau, M. Manera, M. Rashkovetskyi, M. Schubnell, M. Vargas-Maga\~na, M. Walther, N. Deiosso, N. Palanque-Delabrouille, O. Alves, O. Lahav, P. Carrilho, P. Doel, P. Martini, P. Taylor, P. Zarrouk, Q. Li, R. Calderon, R. de Belsunce, R. Kehoe, R. Miquel, R. Zhou, S. Ahlen, S. Bailey, S. BenZvi, S. Cole, S. Gontcho A Gontcho, S. Juneau, S. Nadathur, T. Claybaugh, U. Andrade, W. Elbers, W. J. Percival, W. L. Matthewson, Z. Ding, Z. Zhai

arxiv:2504.18464 v2 · 2025-04-25 · astro-ph.CO · gr-qc

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{QK4KAIWBYIQWKQ3GTAXE4V7V73}

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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

On the potential for inhomogeneities to mimic an evolving dark energy

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM

ACT-ing on inflation: Implications of non Bunch-Davies initial condition and reheating on single-field slow roll models

Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum

Measuring neutrino mass in light of ACT DR6 and DESI DR2

Receipt and verification

First computed	2026-07-05T10:56:18.243595Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

82b8a022c1c221654366982e4e57f5fee45724aa387b4b27191b2159bd308d86

Aliases

arxiv: 2504.18464 · arxiv_version: 2504.18464v2 · doi: 10.48550/arxiv.2504.18464 · pith_short_12: QK4KAIWBYIQW · pith_short_16: QK4KAIWBYIQWKQ3G · pith_short_8: QK4KAIWB

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/QK4KAIWBYIQWKQ3GTAXE4V7V73 \
  | 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: 82b8a022c1c221654366982e4e57f5fee45724aa387b4b27191b2159bd308d86

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "e7d97f9b832840882df06005cbedb4ca6175cfb1a69f1c88084a6303ae042b66",
    "cross_cats_sorted": [
      "gr-qc"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2025-04-25T16:20:03Z",
    "title_canon_sha256": "b391d2383bb03edff01a023971eb64e581c53716a89075b7dc5e2ebb37ad4828"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2504.18464",
    "kind": "arxiv",
    "version": 2
  }
}