Pith Number

pith:O44MIPIV

pith:2019:O44MIPIVWYWNTU4PIKCBJ5W7DF

not attested not anchored not stored refs pending

Planck 2018 results. V. CMB power spectra and likelihoods

A. A. Fraisse, A. Challinor, A. De Rosa, A. Ducout, A. Frolov, A. Gruppuso, A. H. Jaffe, A. J. Banday, A. Lasenby, A. Lewis, A. Mangilli, A. Marcos-Caballero, A. Melchiorri, A. Mennella, A. Moneti, A. Moss, A. Renzi, A.-S. Suur-Uski, A. Zacchei, A. Zonca, B. Casaponsa, B. D. Wandelt, B. Partridge, B. P. Crill, B. Ruiz-Granados, B. Van Tent, C. Baccigalupi, C. Burigana, C. Combet, C. R. Lawrence, C. Rosset, C. Sirignano, D. Herranz, D. Maino, D. Molinari, D. Paoletti, D. Scott, D. Tavagnacco, E. Calabrese, E. Di Valentino, E. Franceschi, E. Hivon, E. Keih\"anen, E. Mart\'inez-Gonz\'alez, E. P. S. Shellard, F. Boulanger, F. Cuttaia, F. Elsner, F. Finelli, F. K. Hansen, F. Levrier, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Villa, G. de Zotti, G. Efstathiou, G. Lagache, G. Maggio, G. Morgante, G. Patanchon, G. Polenta, G. Rocha, G. Roudier, G. Sirri, H. C. Chiang, H. K. Eriksen, H. Kurki-Suonio, H. U. N{\o}rgaard-Nielsen, H. V. Peiris, I. K. Wehus, J. A. Rubi\~no-Mart\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Carron, J. Delabrouille, J. D. McEwen, J. E. Gudmundsson, J.-F. Cardoso, J. F. Mac\'ias-P\'erez, J. Gonz\'alez-Nuevo, J. Hamann, J. J. Bock, J. Kim, J.-L. Puget, J.-M. Delouis, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Valiviita, K. Benabed, K. Ganga, K. Kiiveri, K. M. G\'orski, L. D. Spencer, L. Montier, L. Pagano, L. P. L. Colombo, L. Salvati, L. Toffolatti, M.-A. Miville-Desch\^enes, M. Ashdown, M. Ballardini, M. Bersanelli, M. Bucher, M. Douspis, M. Frailis, M. Gerbino, M. Kunz, M. Lattanzi, M. Le Jeune, M. Liguori, M. Lilley, M. L\'opez-Caniego, M. Maris, M. Migliaccio, M. Millea, M. Reinecke, M. Remazeilles, M. Sandri, M. Savelainen, M. Tenti, M. Tomasi, N. Bartolo, N. Krachmalnicoff, N. Mandolesi, N. Mauri, N. Vittorio, O. Dor\'e, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration: N. Aghanim, P. M. Lubin, P. Natoli, P. R. Meinhold, P. Vielva, R. B. Barreiro, R. C. Butler, R. Fernandez-Cobos, R. Keskitalo, R. Sunyaev, R. T. G\'enova-Santos, S. Basak, S. Dusini, S. Galeotta, S. Galli, S. Gratton, S. Matarrese, T. A. En{\ss}lin, T. Ghosh, T. S. Kisner, T. Trombetti, V. Lindholm, V. Pettorino, W. C. Jones, W. Handley, X. Dupac, Y. Akrami, Y. Fantaye, Y. Giraud-H\'eraud, Y.-Z. Ma, Z. Huang

Refined corrections let Planck 2018 use full polarization data and tighten LambdaCDM constraints by 20-30 percent.

arxiv:1907.12875 v2 · 2019-07-30 · astro-ph.CO

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{O44MIPIVWYWNTU4PIKCBJ5W7DF}

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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.

Claims

C1strongest claim

Overall, the legacy Planck CMB likelihoods provide a robust tool for constraining the cosmological model and represent a reference for future CMB observations.

C2weakest assumption

The accuracy of the polarization efficiency (PE) modelling is the main limitation, with residual modelling uncertainties remaining after corrections for temperature-to-polarization leakage and channel calibrations.

C3one line summary

Planck 2018 likelihoods incorporate improved polarization modeling and simulations to deliver 20-30% tighter Lambda-CDM constraints than temperature-only analyses while maintaining consistency below 0.5 sigma.

Cited by

42 papers in Pith

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MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys

Generalized neutrino isocurvature

The CMB Cold Spot under the lens II: Lensing signatures in polarization and cosmic texture footprints

Signatures of Modified Gravity Below $\mathcal{O}(10)$ Mpc in a Dynamical Dark Energy Background

Receipt and verification

First computed	2026-05-17T23:38:50.029716Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

7738c43d15b62cd9d38f428414f6df1940975bdf322e2989c3630863128e2842

Aliases

arxiv: 1907.12875 · arxiv_version: 1907.12875v2 · doi: 10.48550/arxiv.1907.12875 · pith_short_12: O44MIPIVWYWN · pith_short_16: O44MIPIVWYWNTU4P · pith_short_8: O44MIPIV

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/O44MIPIVWYWNTU4PIKCBJ5W7DF \
  | 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: 7738c43d15b62cd9d38f428414f6df1940975bdf322e2989c3630863128e2842

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "939c83bbafe15ba83e510b28d3754a4f01df629f20fceca1b4166363f138c5c2",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2019-07-30T13:11:32Z",
    "title_canon_sha256": "11607f336c01dfe0b57246f68ec75a5ee76275457bc00f0a5a1ef24f04d32ca9"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1907.12875",
    "kind": "arxiv",
    "version": 2
  }
}