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Title: Planck 2018 results. VI. Cosmological parameters

Abstract

In this paper, we present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with higher precision, leading to significant gains in the precision of other correlated parameters. Improved modelling of the small-scale polarization leads to more robust constraints on many parameters, with residual modelling uncertainties estimated to affect them only at the 0.5σ level. We find good consistency with the standard spatially-flat 6-parameter ΛCDM cosmology having a power-law spectrum of adiabatic scalar perturbations (denoted “base ΛCDM” in this paper), from polarization, temperature, and lensing, separately and in combination. A combined analysis gives dark matter density Ωch2 = 0.120 ± 0.001, baryon density Ωbh2 = 0.0224 ± 0.0001, scalar spectral index ns = 0.965 ± 0.004, and optical depth τ = 0.054 ± 0.007 (in this abstract we quote 68% confidence regions on measured parameters and 95% on upper limits). The angular acoustic scale is measured to 0.03% precision, with 100θ* = 1.0411 ± 0.0003. These results are only weakly dependent on themore » cosmological model and remain stable, with somewhat increased errors, in many commonly considered extensions. Assuming the base-ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4 ± 0.5) km s–1 Mpc–1; matter density parameter Ωm = 0.315 ± 0.007; and matter fluctuation amplitude σ8 = 0.811 ± 0.006. We find no compelling evidence for extensions to the base-ΛCDM model. Combining with baryon acoustic oscillation (BAO) measurements (and considering single-parameter extensions) we constrain the effective extra relativistic degrees of freedom to be Neff = 2.99 ± 0.17, in agreement with the Standard Model prediction Neff = 3.046, and find that the neutrino mass is tightly constrained to Σmν < 0.12 eV. The CMB spectra continue to prefer higher lensing amplitudes than predicted in base ΛCDM at over 2σ, which pulls some parameters that affect the lensing amplitude away from the ΛCDM model; however, this is not supported by the lensing reconstruction or (in models that also change the background geometry) BAO data. The joint constraint with BAO measurements on spatial curvature is consistent with a flat universe, ΩK = 0.001 ± 0.002. Also combining with Type Ia supernovae (SNe), the dark-energy equation of state parameter is measured to be w0 = –1.03 ± 0.03, consistent with a cosmological constant. We find no evidence for deviations from a purely power-law primordial spectrum, and combining with data from BAO, BICEP2, and Keck Array data, we place a limit on the tensor-to-scalar ratio r0.002 < 0.06. Standard big-bang nucleosynthesis predictions for the helium and deuterium abundances for the base-ΛCDM cosmology are in excellent agreement with observations. The Planck base-ΛCDM results are in good agreement with BAO, SNe, and some galaxy lensing observations, but in slight tension with the Dark Energy Survey’s combined-probe results including galaxy clustering (which prefers lower fluctuation amplitudes or matter density parameters), and in significant, 3.6σ, tension with local measurements of the Hubble constant (which prefer a higher value). Simple model extensions that can partially resolve these tensions are not favoured by the Planck data.« less

Authors:
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Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC); European Research Council (ERC); National Aeronautics and Space Administration (NASA)
Contributing Org.:
Planck Collaboration
OSTI Identifier:
1676387
Grant/Contract Number:  
AC02-05CH11231; 616170; 725456
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 641; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Cosmology: observations; Cosmology: theory; Cosmic background radiation; cosmological parameters

Citation Formats

Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Battye, R., Benabed, K., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bock, J. J., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Carron, J., Challinor, A., Chiang, H. C., Chluba, J., Colombo, L. L., Combet, C., Contreras, D., Crill, B. P., Cuttaia, F., de Bernardis, P., de Zotti, G., Delabrouille, J., Delouis, J. -M., Di Valentino, E., Diego, J. M., Doré, O., Douspis, M., Ducout, A., Dupac, X., Dusini, S., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Fantaye, Y., Farhang, M., Fergusson, J., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A. A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R. T., Gerbino, M., Ghosh, T., González-Nuevo, J., Górski, K. M., Gratton, S., Gruppuso, A., Gudmundsson, J. E., Hamann, J., Handley, W., Hansen, F. K., Herranz, D., Hildebrandt, S. R., Hivon, E., Huang, Z., Jaffe, A. H., Jones, W. C., Karakci, A., Keihänen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Knox, L., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Lemos, P., Lesgourgues, J., Levrier, F., Lewis, A., Liguori, M., Lilje, P. B., Lilley, M., Lindholm, V., López-Caniego, M., Lubin, P. M., Ma, Y. -Z., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., Maris, M., Martin, P. G., Martinelli, M., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J. D., Meinhold, P. R., Melchiorri, A., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, M. -A., Molinari, D., Montier, L., Morgante, G., Moss, A., Natoli, P., Nørgaard-Nielsen, H. U., Pagano, L., Paoletti, D., Partridge, B., Patanchon, G., Peiris, H. V., Perrotta, F., Pettorino, V., Piacentini, F., Polastri, L., Polenta, G., Puget, J. -L., Rachen, J. P., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rosset, C., Roudier, G., Rubiño-Martín, J. A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Shellard, E. S., Sirignano, C., Sirri, G., Spencer, L. D., Sunyaev, R., Suur-Uski, A. -S., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Trombetti, T., Valenziano, L., Valiviita, J., Van Tent, B., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wandelt, B. D., Wehus, I. K., White, M., White, S. M., Zacchei, A., and Zonca, A.. Planck 2018 results. VI. Cosmological parameters. United States: N. p., 2020. Web. doi:10.1051/0004-6361/201833910.
Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Battye, R., Benabed, K., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bock, J. J., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Carron, J., Challinor, A., Chiang, H. C., Chluba, J., Colombo, L. L., Combet, C., Contreras, D., Crill, B. P., Cuttaia, F., de Bernardis, P., de Zotti, G., Delabrouille, J., Delouis, J. -M., Di Valentino, E., Diego, J. M., Doré, O., Douspis, M., Ducout, A., Dupac, X., Dusini, S., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Fantaye, Y., Farhang, M., Fergusson, J., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A. A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R. T., Gerbino, M., Ghosh, T., González-Nuevo, J., Górski, K. M., Gratton, S., Gruppuso, A., Gudmundsson, J. E., Hamann, J., Handley, W., Hansen, F. K., Herranz, D., Hildebrandt, S. R., Hivon, E., Huang, Z., Jaffe, A. H., Jones, W. C., Karakci, A., Keihänen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Knox, L., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Lemos, P., Lesgourgues, J., Levrier, F., Lewis, A., Liguori, M., Lilje, P. B., Lilley, M., Lindholm, V., López-Caniego, M., Lubin, P. M., Ma, Y. -Z., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., Maris, M., Martin, P. G., Martinelli, M., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J. D., Meinhold, P. R., Melchiorri, A., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, M. -A., Molinari, D., Montier, L., Morgante, G., Moss, A., Natoli, P., Nørgaard-Nielsen, H. U., Pagano, L., Paoletti, D., Partridge, B., Patanchon, G., Peiris, H. V., Perrotta, F., Pettorino, V., Piacentini, F., Polastri, L., Polenta, G., Puget, J. -L., Rachen, J. P., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rosset, C., Roudier, G., Rubiño-Martín, J. A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Shellard, E. S., Sirignano, C., Sirri, G., Spencer, L. D., Sunyaev, R., Suur-Uski, A. -S., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Trombetti, T., Valenziano, L., Valiviita, J., Van Tent, B., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wandelt, B. D., Wehus, I. K., White, M., White, S. M., Zacchei, A., & Zonca, A.. Planck 2018 results. VI. Cosmological parameters. United States. https://doi.org/10.1051/0004-6361/201833910
Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Battye, R., Benabed, K., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bock, J. J., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Carron, J., Challinor, A., Chiang, H. C., Chluba, J., Colombo, L. L., Combet, C., Contreras, D., Crill, B. P., Cuttaia, F., de Bernardis, P., de Zotti, G., Delabrouille, J., Delouis, J. -M., Di Valentino, E., Diego, J. M., Doré, O., Douspis, M., Ducout, A., Dupac, X., Dusini, S., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Fantaye, Y., Farhang, M., Fergusson, J., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A. A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R. T., Gerbino, M., Ghosh, T., González-Nuevo, J., Górski, K. M., Gratton, S., Gruppuso, A., Gudmundsson, J. E., Hamann, J., Handley, W., Hansen, F. K., Herranz, D., Hildebrandt, S. R., Hivon, E., Huang, Z., Jaffe, A. H., Jones, W. C., Karakci, A., Keihänen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Knox, L., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Lemos, P., Lesgourgues, J., Levrier, F., Lewis, A., Liguori, M., Lilje, P. B., Lilley, M., Lindholm, V., López-Caniego, M., Lubin, P. M., Ma, Y. -Z., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., Maris, M., Martin, P. G., Martinelli, M., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J. D., Meinhold, P. R., Melchiorri, A., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, M. -A., Molinari, D., Montier, L., Morgante, G., Moss, A., Natoli, P., Nørgaard-Nielsen, H. U., Pagano, L., Paoletti, D., Partridge, B., Patanchon, G., Peiris, H. V., Perrotta, F., Pettorino, V., Piacentini, F., Polastri, L., Polenta, G., Puget, J. -L., Rachen, J. P., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rosset, C., Roudier, G., Rubiño-Martín, J. A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Shellard, E. S., Sirignano, C., Sirri, G., Spencer, L. D., Sunyaev, R., Suur-Uski, A. -S., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Trombetti, T., Valenziano, L., Valiviita, J., Van Tent, B., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wandelt, B. D., Wehus, I. K., White, M., White, S. M., Zacchei, A., and Zonca, A.. Fri . "Planck 2018 results. VI. Cosmological parameters". United States. https://doi.org/10.1051/0004-6361/201833910. https://www.osti.gov/servlets/purl/1676387.
@article{osti_1676387,
title = {Planck 2018 results. VI. Cosmological parameters},
author = {Aghanim, N. and Akrami, Y. and Ashdown, M. and Aumont, J. and Baccigalupi, C. and Ballardini, M. and Banday, A. J. and Barreiro, R. B. and Bartolo, N. and Basak, S. and Battye, R. and Benabed, K. and Bernard, J. -P. and Bersanelli, M. and Bielewicz, P. and Bock, J. J. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Boulanger, F. and Bucher, M. and Burigana, C. and Butler, R. C. and Calabrese, E. and Cardoso, J. -F. and Carron, J. and Challinor, A. and Chiang, H. C. and Chluba, J. and Colombo, L. L. and Combet, C. and Contreras, D. and Crill, B. P. and Cuttaia, F. and de Bernardis, P. and de Zotti, G. and Delabrouille, J. and Delouis, J. -M. and Di Valentino, E. and Diego, J. M. and Doré, O. and Douspis, M. and Ducout, A. and Dupac, X. and Dusini, S. and Efstathiou, G. and Elsner, F. and Enßlin, T. A. and Eriksen, H. K. and Fantaye, Y. and Farhang, M. and Fergusson, J. and Fernandez-Cobos, R. and Finelli, F. and Forastieri, F. and Frailis, M. and Fraisse, A. A. and Franceschi, E. and Frolov, A. and Galeotta, S. and Galli, S. and Ganga, K. and Génova-Santos, R. T. and Gerbino, M. and Ghosh, T. and González-Nuevo, J. and Górski, K. M. and Gratton, S. and Gruppuso, A. and Gudmundsson, J. E. and Hamann, J. and Handley, W. and Hansen, F. K. and Herranz, D. and Hildebrandt, S. R. and Hivon, E. and Huang, Z. and Jaffe, A. H. and Jones, W. C. and Karakci, A. and Keihänen, E. and Keskitalo, R. and Kiiveri, K. and Kim, J. and Kisner, T. S. and Knox, L. and Krachmalnicoff, N. and Kunz, M. and Kurki-Suonio, H. and Lagache, G. and Lamarre, J. -M. and Lasenby, A. and Lattanzi, M. and Lawrence, C. R. and Le Jeune, M. and Lemos, P. and Lesgourgues, J. and Levrier, F. and Lewis, A. and Liguori, M. and Lilje, P. B. and Lilley, M. and Lindholm, V. and López-Caniego, M. and Lubin, P. M. and Ma, Y. -Z. and Macías-Pérez, J. F. and Maggio, G. and Maino, D. and Mandolesi, N. and Mangilli, A. and Marcos-Caballero, A. and Maris, M. and Martin, P. G. and Martinelli, M. and Martínez-González, E. and Matarrese, S. and Mauri, N. and McEwen, J. D. and Meinhold, P. R. and Melchiorri, A. and Mennella, A. and Migliaccio, M. and Millea, M. and Mitra, S. and Miville-Deschênes, M. -A. and Molinari, D. and Montier, L. and Morgante, G. and Moss, A. and Natoli, P. and Nørgaard-Nielsen, H. U. and Pagano, L. and Paoletti, D. and Partridge, B. and Patanchon, G. and Peiris, H. V. and Perrotta, F. and Pettorino, V. and Piacentini, F. and Polastri, L. and Polenta, G. and Puget, J. -L. and Rachen, J. P. and Reinecke, M. and Remazeilles, M. and Renzi, A. and Rocha, G. and Rosset, C. and Roudier, G. and Rubiño-Martín, J. A. and Ruiz-Granados, B. and Salvati, L. and Sandri, M. and Savelainen, M. and Scott, D. and Shellard, E. S. and Sirignano, C. and Sirri, G. and Spencer, L. D. and Sunyaev, R. and Suur-Uski, A. -S. and Tauber, J. A. and Tavagnacco, D. and Tenti, M. and Toffolatti, L. and Tomasi, M. and Trombetti, T. and Valenziano, L. and Valiviita, J. and Van Tent, B. and Vibert, L. and Vielva, P. and Villa, F. and Vittorio, N. and Wandelt, B. D. and Wehus, I. K. and White, M. and White, S. M. and Zacchei, A. and Zonca, A.},
abstractNote = {In this paper, we present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with higher precision, leading to significant gains in the precision of other correlated parameters. Improved modelling of the small-scale polarization leads to more robust constraints on many parameters, with residual modelling uncertainties estimated to affect them only at the 0.5σ level. We find good consistency with the standard spatially-flat 6-parameter ΛCDM cosmology having a power-law spectrum of adiabatic scalar perturbations (denoted “base ΛCDM” in this paper), from polarization, temperature, and lensing, separately and in combination. A combined analysis gives dark matter density Ωch2 = 0.120 ± 0.001, baryon density Ωbh2 = 0.0224 ± 0.0001, scalar spectral index ns = 0.965 ± 0.004, and optical depth τ = 0.054 ± 0.007 (in this abstract we quote 68% confidence regions on measured parameters and 95% on upper limits). The angular acoustic scale is measured to 0.03% precision, with 100θ* = 1.0411 ± 0.0003. These results are only weakly dependent on the cosmological model and remain stable, with somewhat increased errors, in many commonly considered extensions. Assuming the base-ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4 ± 0.5) km s–1 Mpc–1; matter density parameter Ωm = 0.315 ± 0.007; and matter fluctuation amplitude σ8 = 0.811 ± 0.006. We find no compelling evidence for extensions to the base-ΛCDM model. Combining with baryon acoustic oscillation (BAO) measurements (and considering single-parameter extensions) we constrain the effective extra relativistic degrees of freedom to be Neff = 2.99 ± 0.17, in agreement with the Standard Model prediction Neff = 3.046, and find that the neutrino mass is tightly constrained to Σmν < 0.12 eV. The CMB spectra continue to prefer higher lensing amplitudes than predicted in base ΛCDM at over 2σ, which pulls some parameters that affect the lensing amplitude away from the ΛCDM model; however, this is not supported by the lensing reconstruction or (in models that also change the background geometry) BAO data. The joint constraint with BAO measurements on spatial curvature is consistent with a flat universe, ΩK = 0.001 ± 0.002. Also combining with Type Ia supernovae (SNe), the dark-energy equation of state parameter is measured to be w0 = –1.03 ± 0.03, consistent with a cosmological constant. We find no evidence for deviations from a purely power-law primordial spectrum, and combining with data from BAO, BICEP2, and Keck Array data, we place a limit on the tensor-to-scalar ratio r0.002 < 0.06. Standard big-bang nucleosynthesis predictions for the helium and deuterium abundances for the base-ΛCDM cosmology are in excellent agreement with observations. The Planck base-ΛCDM results are in good agreement with BAO, SNe, and some galaxy lensing observations, but in slight tension with the Dark Energy Survey’s combined-probe results including galaxy clustering (which prefers lower fluctuation amplitudes or matter density parameters), and in significant, 3.6σ, tension with local measurements of the Hubble constant (which prefer a higher value). Simple model extensions that can partially resolve these tensions are not favoured by the Planck data.},
doi = {10.1051/0004-6361/201833910},
journal = {Astronomy and Astrophysics},
number = ,
volume = 641,
place = {United States},
year = {2020},
month = {9}
}

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Baryon acoustic oscillations from the complete SDSS-III Ly α -quasar cross-correlation function at z = 2.4
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Sterile neutrinos with secret interactions—lasting friendship with cosmology
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The Atacama Cosmology Telescope: two-season ACTPol spectra and parameters
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Planck 2018 results: IV. Diffuse component separation
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Was there an early reionization component in our universe?
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Survey geometry and the internal consistency of recent cosmic shear measurements
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Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters
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Planck 2015 results : XVII. Constraints on primordial non-Gaussianity
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Clarifying the Hubble constant tension with a Bayesian hierarchical model of the local distance ladder
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Planck 2015 results : XIII. Cosmological parameters
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Planck 2015 results : XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
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Primeval Adiabatic Perturbation in an Expanding Universe
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Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7
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Relic neutrino decoupling including flavour oscillations
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Planck 2018 results: XII. Galactic astrophysics using polarized dust emission
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Planck 2018 results: X. Constraints on inflation
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How well do we understand cosmological recombination?
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On the Nature of Hydrostatic Equilibrium in Galaxy Clusters
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Model‐Independent Constraints on Reionization from Large‐Scale Cosmic Microwave Background Polarization
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Dark Energy after GW170817 and GRB170817A
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The Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fraction Using Ly α Emission from Galaxies
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Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
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Dark Energy After GW170817: Dead Ends and the Road Ahead
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Constraints on neutrino masses from Lyman-alpha forest power spectrum with BOSS and XQ-100
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A New Calculation of the Recombination Epoch
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Witnessing the reionization history using Cosmic Microwave Background observation from Planck
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Acoustic dark energy: Potential conversion of the Hubble tension
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Baryon acoustic oscillations in the Ly α forest of BOSS DR11 quasars
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Sterile Neutrino Constraints from the STEREO Experiment with 66 Days of Reactor-On Data
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Changing the Bayesian prior: Absolute neutrino mass constraints in nonlocal gravity
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Coupled quintessence
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Hungary rewards highly cited scientists with bonus grants
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Weak gravitational lensing
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Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV
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Inflationary paradigm in trouble after Planck2013
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Systematic uncertainties in constraining dark matter annihilation from the cosmic microwave background
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The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at z ∼ 1.4
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The Primordial Lithium Problem
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Sterile neutrinos as dark matter
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Modeling the Radio Background from the First Black Holes at Cosmic Dawn: Implications for the 21 cm Absorption Amplitude
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Crossing the phantom divide with parametrized post-Friedmann dark energy
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Weak gravitational lensing of the CMB
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Planck data reconsidered
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Pseudoscalar—sterile neutrino interactions: reconciling the cosmos with neutrino oscillations
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QUANTIFYING DISCORDANCE IN THE 2015 PLANCK CMB SPECTRUM
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Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman-α
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
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Implication of the Proton-Deuteron Radiative Capture for Big Bang Nucleosynthesis
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Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays
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Dark matter and pulsar model constraints from Galactic Center Fermi-LAT gamma-ray observations
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Constraints on Perturbations to the Recombination History from Measurements of the Cosmic Microwave Background Damping tail
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Towards a cosmological neutrino mass detection
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A tale of tails: Dark matter interpretations of the Fermi GeV excess in light of background model systematics
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Bounds on very low reheating scenarios after Planck
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HyRec: A fast and highly accurate primordial hydrogen and helium recombination code
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Evidence for dark matter interactions in cosmological precision data?
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Signature of Gravity Waves in the Polarization of the Microwave Background
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Scalar-tensor theories and modified gravity in the wake of GW170817
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Prospects for Resolving the Hubble Constant Tension with Standard Sirens
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The WiggleZ Dark Energy Survey: improved distance measurements to z = 1 with reconstruction of the baryonic acoustic feature
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Standard Rulers, Candles, and Clocks from the Low-Redshift Universe
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The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes
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Planck 2013 results. XXII. Constraints on inflation
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Astrophysical and dark matter interpretations of extended gamma-ray emission from the Galactic Center
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Determining the Initial Helium Abundance of the sun
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Self-accelerating universe in scalar-tensor theories after GW170817
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Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
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White dwarfs and revelations
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Probing Gravity at Cosmological Scales by Measurements which Test the Relationship between Gravitational Lensing and Matter Overdensity
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Interacting dark sector and precision cosmology
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Ultrafast effective multilevel atom method for primordial hydrogen recombination
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Dark energy, α-attractors, and large-scale structure surveys
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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Precision Measures of the Primordial Abundance of Deuterium
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Joint analysis of CMB temperature and lensing-reconstruction power spectra
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How Exactly Did the Universe Become Neutral?
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The WiggleZ Dark Energy Survey: Final data release and cosmological results
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The effective field theory of dark energy
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Novel Dark Matter Constraints from Antiprotons in Light of AMS-02
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Planck 2013 results. XVII. Gravitational lensing by large-scale structure
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An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5
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Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
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Planck 2015 results : XX. Constraints on inflation
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Reducing the H 0 and σ 8 tensions with dark matter-neutrino interactions
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Sensitivity projections for dark matter searches with the Fermi large area telescope
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Model-independent ν ¯ e short-baseline oscillations from reactor spectral ratios
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Vector-Metric Theory of Gravity
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Induced two-photon decay of the 2s level and the rate of cosmological hydrogen recombination
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Cosmological constraints on the neutron lifetime
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Probing nuclear rates with Planck and BICEP2
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Underground Study of Big Bang Nucleosynthesis in the Precision Era of Cosmology
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Minimal supergravity models of inflation
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Characterizing the epoch of reionization with the small-scale CMB: Constraints on the optical depth and duration
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KiDS+VIKING-450: Cosmic shear tomography with optical and infrared data
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Superconformal inflationary α-attractors
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Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies
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Can dark energy evolve to the phantom?
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Power spectra based Planck constraints on compensated isocurvature, and forecasts for LiteBIRD and CORE space missions
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PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
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Final results of the search for νμ → νe oscillations with the OPERA detector in the CNGS beam
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Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of Sptpol data
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The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant: 6dFGS: BAOs and the local Hubble constant
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Estimating reaction rates and uncertainties for primordial nucleosynthesis
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Relieving tensions related to the lensing of the cosmic microwave background temperature power spectra
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THE MEGAMASER COSMOLOGY PROJECT. VIII. A GEOMETRIC DISTANCE TO NGC 5765b
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Essential building blocks of dark energy
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Massive neutrinos and cosmology
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PArthENoPE: Public algorithm evaluating the nucleosynthesis of primordial elements
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Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
journal, July 2018

  • Riess, Adam G.; Casertano, Stefano; Yuan, Wenlong
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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2
journal, October 2017

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Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
journal, March 2017

  • Alam, Shadab; Ata, Metin; Bailey, Stephen
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Planck 2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts
journal, October 2014


CMB polarization can constrain cosmology better than CMB temperature
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Anisotropic Stress as a Signature of Nonstandard Propagation of Gravitational Waves
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Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
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First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic Results
journal, September 2003

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Relic neutrino decoupling with flavour oscillations revisited
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CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products
journal, June 2013

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Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure
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Constraining Cosmological Parameters Based on Relative Galaxy Ages
journal, July 2002

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Early Dark Energy can Resolve the Hubble Tension
journal, June 2019


Breaking a dark degeneracy with gravitational waves
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Microwave Background Constraints on Cosmological Parameters
journal, October 1997

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Cosmological parameters from WMAP 5-year temperature maps
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Weighing the giants – IV. Cosmology and neutrino mass
journal, November 2014

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The Atacama Cosmology Telescope: cosmological parameters from three seasons of data
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Dark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data
journal, July 2018

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Measuring the dark side (with weak lensing)
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Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
journal, August 2019

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Testing gravity with CAMB and CosmoMC
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Crossing the phantom divide
journal, December 2006


Extended Limber approximation
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Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy
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On the Problem of Initial Conditions for Inflation
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THE MEGAMASER COSMOLOGY PROJECT. V. AN ANGULAR-DIAMETER DISTANCE TO NGC 6264 AT 140 Mpc
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Cosmological parameters from CMB and other data: A Monte Carlo approach
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Full covariance of CMB and lensing reconstruction power spectra
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The Megamaser Cosmology Project. iv. a Direct Measurement of the Hubble Constant from ugc 3789
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New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope : Implications for the Hubble Constant
journal, March 2018

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First Search for Short-Baseline Neutrino Oscillations at HFIR with PROSPECT
journal, December 2018


Effective description of higher-order scalar-tensor theories
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Tensions between direct measurements of the lens power spectrum from Planck data
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Concordance and discordance in cosmology
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Effect of physical assumptions on the calculation of microwave background anisotropies
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The 6dF Galaxy Survey: z≈ 0 measurements of the growth rate and σ8: 6dFGS: z≈ 0 measurements of fσ8 and σ8
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Improved Determination of the Neutron Lifetime
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Stable clustering, the halo model and non-linear cosmological power spectra
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Current unknowns in the three-neutrino framework
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Internal delensing of Planck CMB temperature and polarization
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Planck 2018 results: V. CMB power spectra and likelihoods
journal, September 2020


Searching for dark matter in the CMB: A compact parametrization of energy injection from new physics
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Planck pre-launch status: High Frequency Instrument polarization calibration
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Calculation of the axion mass based on high-temperature lattice quantum chromodynamics
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Implications of Planck2015 for inflationary, ekpyrotic and anamorphic bouncing cosmologies
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Measurement of CIB power spectra over large sky areas from Planck HFI maps
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NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS
journal, September 2013

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Simultaneous constraints on the growth of structure and cosmic expansion from the multipole power spectra of the SDSS DR7 LRG sample
journal, February 2014

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Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
journal, February 2020

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Joint Analysis of BICEP2/ Keck Array and Planck Data
journal, March 2015


QuickPol: Fast calculation of effective beam matrices for CMB polarization
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Cosmic Microwave Background Constraints on the Duration and Timing of Reionization from the South pole Telescope
journal, August 2012


KiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
journal, November 2016

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Testing cosmological structure formation using redshift-space distortions
journal, February 2009


The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structure at 0.5 <
journal, July 2017


Dark Energy Survey year 1 results: Galaxy clustering for combined probes
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A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3
journal, March 2011


Cosmological Parameter Uncertainties from Salt-Ii type ia Supernova Light Curve Models
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Weak lensing of the CMB
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Dark Energy Survey year 1 results: Galaxy-galaxy lensing
journal, August 2018


The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Fourier space
journal, September 2016

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KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear
journal, May 2020


The Atacama Cosmology Telescope: dynamical masses for 44 SZ-selected galaxy clusters over 755 square degrees
journal, May 2016

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Planck intermediate results : XLVII.
journal, December 2016


The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: observational systematics and baryon acoustic oscillations in the correlation function
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Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
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The Atacama Cosmology Telescope: CMB polarization at 200 < ℓ < 9000
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RCSLenS: The Red Cluster Sequence Lensing Survey
journal, August 2016

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The Extended Northern ROSAT Galaxy Cluster Survey (NORAS II). I. Survey Construction and First Results
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Improved photometric calibration of the SNLS and the SDSS supernova surveys
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A two per cent Hubble constant measurement from standard sirens within five years
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Testing modified gravity with Planck: The case of coupled dark energy
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Insensitivity of the distance ladder Hubble constant determination to Cepheid calibration modelling choices
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Finding Horndeski theories with Einstein gravity limits
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Neutron lifetime measurements with a large gravitational trap for ultracold neutrons
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A 2.4% Determination of the Local Value of the Hubble Constant
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Baryon acoustic oscillations at z = 2.34 from the correlations of Ly α absorption in eBOSS DR14
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CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey: CFHTLenS
journal, October 2012

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Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear
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Status of neutrino oscillations 2018: 3 σ hint for normal mass ordering and improved CP sensitivity
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Planck 2018 results: II. Low Frequency Instrument data processing
journal, September 2020


Detecting Patchy Reionization in the Cosmic Microwave Background
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Calibration of the Tip of the Red Giant Branch
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Complete reionization constraints from Planck 2015 polarization
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Transforming gravity: From derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian
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Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects
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Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
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Nonlocal gravity. Conceptual aspects and cosmological predictions
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Testing ΛCDM at the lowest redshifts with SN Ia and galaxy velocities
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Robust weak-lensing mass calibration of Planck galaxy clusters
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New Class of Consistent Scalar-Tensor Theories
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Maximum-Entropy Priors with Derived Parameters in a Specified Distribution
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Assessing Consistency between WMAP 9 Year and Planck 2015 Temperature Power Spectra
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Revising the Halofit Model for the Nonlinear Matter Power Spectrum
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The effective field theory of inflation
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Calibrating the Planck cluster mass scale with CLASH
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Effective field theory of cosmic acceleration: Constraining dark energy with CMB data
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions
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Searching for modified growth patterns with tomographic surveys
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Constraints on Oscillation Parameters from ν e Appearance and ν μ Disappearance in NOvA
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Model-independent implications of the , cosmic ray spectra on properties of Dark Matter
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Cosmological Constraints from Galaxy Clusters in the 2500 Square-Degree Spt-Sz Survey
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Cosmic microwave background constraints in light of priors over reionization histories
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Quasar-Lyman α forest cross-correlation from BOSS DR11: Baryon Acoustic Oscillations
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Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium
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Rapid He II->He I recombination and radiation arising from this process
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Secondary Cosmic Microwave Background Anisotropies in a Universe Reionized in Patches
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A tale of two modes: neutrino free-streaming in the early universe
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Inflationary versus reionization features from Planck 2015 data
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Imperfect dark energy from kinetic gravity braiding
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The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
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Baryon acoustic oscillations from the cross-correlation of Ly α absorption and quasars in eBOSS DR14
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The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations at Redshift of 0.72 with the DR14 Luminous Red Galaxy Sample
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The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z < 1 : WiggleZ Survey: expansion history
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Dark Energy Survey Year 1 results: measurement of the baryon acoustic oscillation scale in the distribution of galaxies to redshift 1
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Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces
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Unity of Cosmological Inflation Attractors
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REIONIZATION AFTER PLANCK : THE DERIVED GROWTH OF THE COSMIC IONIZING EMISSIVITY NOW MATCHES THE GROWTH OF THE GALAXY UV LUMINOSITY DENSITY
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Bayesian Estimation of Thermonuclear Reaction Rates
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KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering
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Inflationary paradigm after Planck 2013
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Primordial helium recombination. I. Feedback, line transfer, and continuum opacity
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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
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A Measurement of the Cosmic Microwave Background Damping tail from the 2500-Square-Degree Spt-Sz Survey
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Planck 2015 results : XV. Gravitational lensing
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An evolution free test for non-zero cosmological constant
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Parameter constraints for flat cosmologies from cosmic microwave background and 2dFGRS power spectra
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Planck 2018 results: IX. Constraints on primordial non-Gaussianity
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The trouble with H 0
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Electromagnetic structure of A=2 and 3 nuclei and the nuclear current operator
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Comparison of cosmological Boltzmann codes: Are we ready for high precision cosmology?
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A Measurement of Secondary Cosmic Microwave Background Anisotropies from the 2500 Square-Degree Spt-Sz Survey
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Linear and non-linear Modified Gravity forecasts with future surveys
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The effective theory of quintessence: the w < −1 side unveiled
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A blinded determination of H0 from low-redshift Type Ia supernovae, calibrated by Cepheid variables
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The characterization of the gamma-ray signal from the central Milky Way: A case for annihilating dark matter
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H0 revisited
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Cosmic microwave weak lensing data as a test for the dark universe
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SUPERCAL: CROSS-CALIBRATION OF MULTIPLE PHOTOMETRIC SYSTEMS TO IMPROVE COSMOLOGICAL MEASUREMENTS WITH TYPE Ia SUPERNOVAE
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CMB signatures of metal-free star formation and Planck 2015 polarization data
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Planck 2015 results : XIV. Dark energy and modified gravity
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The effects of He I λ10830 on helium abundance determinations
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Demonstration of Cosmic Microwave Background Delensing Using the Cosmic Infrared Background
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MontePython 3: Boosted MCMC sampler and other features
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Constraints on Primordial Gravitational Waves Using P l a n c k , WMAP, and New BICEP2/ K e c k Observations through the 2015 Season
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Planck 2018 results: XI. Polarized dust foregrounds
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Exotic energy injection with ExoCLASS : application to the Higgs portal model and evaporating black holes
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The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications
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Probing the Reionization History of the Universe using the Cosmic Microwave Background Polarization
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A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
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Model-independent reionization observables in the CMB
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Model selection applied to reconstruction of the Primordial Power Spectrum
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Statistics of cosmic microwave background polarization
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H 0 from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
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Efficient sampling of fast and slow cosmological parameters
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Can active-sterile neutrino oscillations lead to chaotic behavior of the cosmological lepton asymmetry?
journal, April 2013

  • Hannestad, Steen; Hansen, Rasmus Sloth; Tram, Thomas
  • Journal of Cosmology and Astroparticle Physics, Vol. 2013, Issue 04
  • DOI: 10.1088/1475-7516/2013/04/032

A new determination of the primordial He abundance using the He i λ10830 Å emission line: cosmological implications
journal, September 2014

  • Izotov, Y. I.; Thuan, T. X.; Guseva, N. G.
  • Monthly Notices of the Royal Astronomical Society, Vol. 445, Issue 1
  • DOI: 10.1093/mnras/stu1771

Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
journal, December 2016

  • Achour, J. Ben; Crisostomi, M.; Koyama, K.
  • Journal of High Energy Physics, Vol. 2016, Issue 12
  • DOI: 10.1007/JHEP12(2016)100

Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
journal, August 2014


Works referencing / citing this record:

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Extreme starlight polarization in a region with highly polarized dust emission
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Re-evaluating evidence for Hawking points in the CMB
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The flickering nuclear activity of Fornax A
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CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope
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  • Basu, Aritra; Schwarz, Dominik J.; Klöckner, Hans-Rainer
  • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 2
  • DOI: 10.1093/mnras/stz1637

Local Bubble contribution to the 353-GHz dust polarized emission
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Reionization optical depth determination from Planck HFI data with ten percent accuracy
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