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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. 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., & 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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Planck 2015 results : XIII. Cosmological parameters
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Towards a cosmological neutrino mass detection
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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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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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Vector-Metric Theory of Gravity
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Minimal supergravity models of inflation
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PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
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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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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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Ghost-free massive gravity with a general reference metric
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  • Hassan, S. F.; Rosen, Rachel A.; Schmidt-May, Angnis
  • Journal of High Energy Physics, Vol. 2012, Issue 2
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Massive neutrinos and cosmology
journal, July 2006


PArthENoPE: Public algorithm evaluating the nucleosynthesis of primordial elements
journal, June 2008


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
  • The Astrophysical Journal, Vol. 861, Issue 2
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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

  • Ata, Metin; Baumgarten, Falk; Bautista, Julian
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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
journal, September 2014


Anisotropic Stress as a Signature of Nonstandard Propagation of Gravitational Waves
journal, November 2014


Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
journal, July 2014


First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic Results
journal, September 2003

  • Bennett, C. L.; Halpern, M.; Hinshaw, G.
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Relic neutrino decoupling with flavour oscillations revisited
journal, July 2016


CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products
journal, June 2013

  • Erben, T.; Hildebrandt, H.; Miller, L.
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Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure
journal, October 2013

  • Blake, Chris; Baldry, I. K.; Bland-Hawthorn, J.
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Constraining Cosmological Parameters Based on Relative Galaxy Ages
journal, July 2002

  • Jimenez, Raul; Loeb, Abraham
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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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Significant Excess of Electronlike Events in the MiniBooNE Short-Baseline Neutrino Experiment
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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
journal, October 2013

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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)
journal, April 2008

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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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  • Journal of Cosmology and Astroparticle Physics, Vol. 2011, Issue 08
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Crossing the phantom divide
journal, December 2006


Extended Limber approximation
journal, December 2008


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
journal, April 2013


New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope : Implications for the Hubble Constant
journal, March 2018

  • Riess, Adam G.; Casertano, Stefano; Yuan, Wenlong
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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
journal, May 2017

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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
journal, November 1995


The 6dF Galaxy Survey: z≈ 0 measurements of the growth rate and σ8: 6dFGS: z≈ 0 measurements of fσ8 and σ8
journal, June 2012


Improved Determination of the Neutron Lifetime
journal, November 2013


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
journal, December 2016

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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
journal, January 2017


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
journal, August 2018


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
journal, June 2010

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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
journal, March 2019

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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
journal, April 2017

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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
journal, October 2018


Testing modified gravity with Planck: The case of coupled dark energy
journal, September 2013


Insensitivity of the distance ladder Hubble constant determination to Cepheid calibration modelling choices
journal, March 2018

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Finding Horndeski theories with Einstein gravity limits
journal, November 2016

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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
journal, July 2016

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Baryon acoustic oscillations at z = 2.34 from the correlations of Ly α absorption in eBOSS DR14
journal, September 2019

  • de Sainte Agathe, Victoria; Balland, Christophe; du Mas des Bourboux, Hélion
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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
journal, August 2018


Status of neutrino oscillations 2018: 3 σ hint for normal mass ordering and improved CP sensitivity
journal, July 2018


Planck 2018 results: II. Low Frequency Instrument data processing
journal, September 2020


Detecting Patchy Reionization in the Cosmic Microwave Background
journal, July 2017


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
journal, October 2018

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Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
journal, August 2018


Nonlocal gravity. Conceptual aspects and cosmological predictions
journal, March 2018

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Testing ΛCDM at the lowest redshifts with SN Ia and galaxy velocities
journal, May 2017

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Robust weak-lensing mass calibration of Planck galaxy clusters
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New Class of Consistent Scalar-Tensor Theories
journal, May 2015


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
journal, October 2007

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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
journal, December 1998

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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
journal, August 2019

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Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos
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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
journal, April 2015


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
journal, September 2016


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
journal, June 2012

  • Vázquez, J. Alberto; Bridges, M.; Hobson, M. P.
  • Journal of Cosmology and Astroparticle Physics, Vol. 2012, Issue 06
  • DOI: 10.1088/1475-7516/2012/06/006

Statistics of cosmic microwave background polarization
journal, June 1997

  • Kamionkowski, Marc; Kosowsky, Arthur; Stebbins, Albert
  • Physical Review D, Vol. 55, Issue 12
  • DOI: 10.1103/PhysRevD.55.7368

H 0 from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
journal, April 2018


Efficient sampling of fast and slow cosmological parameters
journal, May 2013


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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    • 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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