Cited by 84Cosmology and Gravitation TheoriesDark Matter and Cosmic PhenomenaGalaxies: Formation, Evolution, Phenomena

Constraints on ΛCDM extensions from the SPT-3G 2018 EE and TE power spectra

Open access
Balkenhol, L., Dutcher, D., Ade, P. A. R., Ahmed, Z., Anderes, E., Anderson, A. J., Archipley, M., Avva, J. S. +113 more·2021·Physical Review D

Abstract

The authors present constraints on cosmological models obtained by using state-of-the-art methods on data from the South Pole Telescope (SPT-3G) experiment. Apart from several incremental improvements, the results are in general consistent with those obtained from other data sets and other experiments. In particular, the authors set the tightest constraint on the Hubble constant, ${H}_{0}$, from CMB power spectra to date, which is in $4.1\ensuremath{\sigma}$ tension with the most precise distance-ladder-based measurement of ${H}_{0}$.

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1103/physrevd.104.083509

Cites

54 of 54 references verified0 citation errors · 0 not checkable

Statistics

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Cites

Flagged first, then by citations

Research works printed but not linked: 2

  1. Dutcher, D., Balkenhol, L., Ade, P. A. R., et al. Mea- surements of the E-Mode Polarization and Temperature- E-Mode Correlation of the CMB from SPT-3G 2018 Data. 2021, arXiv e-prints, arXiv:2101.01684. https: //arxiv.org/abs/2101.01684 · arXiv
  2. Freedman, W. L., Madore, B. F., Hatt, D., Hoyt, T. J., Jang, I.-S., Beaton, R. L., Burns, C. R., Lee, M. G., Monson, A. J., Neeley, J. R., Phillips, M. M., Rich, J. A., & Seibert, M. The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch. 2019, arXiv e-prints, arXiv:1907.05922. https: //arxiv.org/abs/1907.05922 · arXiv

Cited by

Sorted by citations

Authors
Balkenhol, L., Dutcher, D., Ade, P. A. R., Ahmed, Z., Anderes, E., Anderson, A. J., Archipley, M., Avva, J. S., Aylor, K., Barry, P. S., Basu Thakur, R., Benabed, K., Bender, A. N., Benson, B. A., Bianchini, F., Bleem, L. E., Bouchet, F. R., Bryant, L., Byrum, K., Carlstrom, J. E., Carter, F. W., Cecil, T. W., Chang, C. L., Chaubal, P., Chen, G., Cho, H.-M., Chou, T.-L., Cliche, J.-F., Crawford, T. M., Cukierman, A., Daley, C., de Haan, T., Denison, E. V., Dibert, K., Ding, J., Dobbs, M. A., Everett, W., Feng, C., Ferguson, K. R., Foster, A., Fu, J., Galli, S., Gambrel, A. E., Gardner, R. W., Goeckner-Wald, N., Gualtieri, R., Guns, S., Gupta, N., Guyser, R., Halverson, N. W., Harke-Hosemann, A. H., Harrington, N. L., Henning, J. W., Hilton, G. C., Hivon, E., Holder, G. P., Holzapfel, W. L., Hood, J. C., Howe, D., Huang, N., Irwin, K. D., Jeong, O. B., Jonas, M., Jones, A., Khaire, T. S., Knox, L., Kofman, A. M., Korman, M., Kubik, D. L., Kuhlmann, S., Kuo, C.-L., Lee, A. T., Leitch, E. M., Lowitz, A. E., Lu, C., Meyer, S. S., Michalik, D., Millea, M., Montgomery, J., Nadolski, A., Natoli, T., Nguyen, H., Noble, G. I., Novosad, V., Omori, Y., Padin, S., Pan, Z., Paschos, P., Pearson, J., Posada, C. M., Prabhu, K., Quan, W., Rahlin, A., Reichardt, C. L., Riebel, D., Riedel, B., Rouble, M., Ruhl, J. E., Sayre, J. T., Schiappucci, E., Shirokoff, E., Smecher, G., Sobrin, J. A., Stark, A. A., Stephen, J., Story, K. T., Suzuki, A., Thompson, K. L., Thorne, B., Tucker, C., Umilta, C., Vale, L. R., Vanderlinde, K., Vieira, J. D., Wang, G., Whitehorn, N., Wu, W. L. K., Yefremenko, V., Yoon, K. W., Young, M. R., & SPT-3G Collaboration
Affiliations
  • The University of Melbourne (AU)
  • University of Chicago (US)
  • Cardiff University (GB)
  • SLAC National Accelerator Laboratory (US)
  • University of California, Davis (US)
  • Fermi National Accelerator Laboratory (US)
  • University of Illinois Urbana-Champaign (US)
  • University of California, Berkeley (US)
  • Argonne National Laboratory (US)
  • Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois, 60637, USA
  • Centre National de la Recherche Scientifique (FR)
  • Trottier Space Institute at McGill (CA)
  • High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
  • National Institute of Standards and Technology (US)
  • Canadian Institute for Advanced Research (CA)
  • University of Colorado Boulder (US)
  • University of California, Los Angeles (US)
  • Case Western Reserve University (US)
  • Kavli Institute for Particle Astrophysics and Cosmology (US)
  • Commonwealth Scientific and Industrial Research Organisation (AU)
  • University of Pennsylvania (US)
  • Lawrence Berkeley National Laboratory (US)
  • California Institute of Technology (US)
  • Three-Speed Logic (Canada) (CA)
  • Center for Astrophysics Harvard & Smithsonian (US)
  • University of Toronto (CA)
Venue
Physical Review D
Published
2021-10-04
Volume
104
Issue
8
Pages
083509
ISSN
  • 2470-0010 (ISSN-L)
  • 2470-0029
OpenAlex
W3137078388
Cited by
84
References
54
Citations by year
2026: 8 · 2025: 18 · 2024: 16 · 2023: 17 · 2022: 21 · 2021: 4
FWCI
7.80
Type
journal article
Language
en
Open access
Locations
  • Physical review. D/Physical review. D. (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
  • eScholarship (California Digital Library) (submittedVersion, cc-by-nc)
  • OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
  • HAL (submittedVersion)
  • ORCA Online Research @Cardiff (Cardiff University) (submittedVersion)
  • Minerva Access (University of Melbourne) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation (PLR-1248097, OPP-1852617, PHY-1125897, AST-0956135, AST-1716965, CSSI-1835865)
  • Kavli Institute for Cosmological Physics, University of Chicago
  • Kavli Foundation
  • Gordon and Betty Moore Foundation (GBMF#947)
  • University of Chicago
  • Argonne National Laboratory
  • U.S. Department of Energy (DE-AC02-06CH11357, DE-AC02-07CH11359, DE-AC02-05CH11231)
  • High Energy Physics
  • Science and Technology Facilities Council
  • Centre National d’Etudes Spatiales
  • Alfred P. Sloan Foundation
  • University of Melbourne
  • Australian Research Council (FT150100074)
  • Natural Sciences and Engineering Research Council of Canada
  • Fonds de recherche du Québec – Nature et technologies
  • Office of Science
  • National Energy Research Scientific Computing Center
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Keywords
South Pole Telescope, SPT-3G, Hubble constant, Hubble tension, cosmological model constraints

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review