| Planck 2018 results-VI. Cosmological parameters N Aghanim, Y Akrami, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 641, A6, 2020 | 14331* | 2020 |
| Planck 2013 results. I. Overview of products and scientific results PAR Ade, N Aghanim, MIR Alves, C Armitage-Caplan, M Arnaud, ... Astronomy & Astrophysics 571, A1, 2014 | 4493* | 2014 |
| Planck 2018 results-X. Constraints on inflation Y Akrami, F Arroja, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 641, A10, 2020 | 3643* | 2020 |
| Planck 2015 results-XX. Constraints on inflation PAR Ade, N Aghanim, M Arnaud, F Arroja, M Ashdown, J Aumont, ... Astronomy & Astrophysics 594, A20, 2016 | 3509* | 2016 |
| Planck 2013 results Planck Collaboration | 2916* | 2014 |
| Planck 2015 results-XVII. Constraints on primordial non-Gaussianity PAR Ade, N Aghanim, M Arnaud, F Arroja, M Ashdown, J Aumont, ... Astronomy & Astrophysics 594, A17, 2016 | 1549* | 2016 |
| Planck 2013 results. XXIII. Isotropy and statistics of the CMB PAR Ade, N Aghanim, C Armitage-Caplan, M Arnaud, M Ashdown, ... Astronomy & Astrophysics 571, A23, 2014 | 1146* | 2014 |
| Erratum: Planck 2018 results: VI. Cosmological parameters (Astronomy and Astrophysics (2020) 641 (A6 N Aghanim, Y Akrami, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 652, 1-3, 2021 | 883 | 2021 |
| Planck 2018 results-V. CMB power spectra and likelihoods N Aghanim, Y Akrami, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 641, A5, 2020 | 825 | 2020 |
| Planck intermediate results-XLVII. Planck constraints on reionization history R Adam, N Aghanim, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 596, A108, 2016 | 543 | 2016 |
| Planck intermediate results-XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth N Aghanim, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 596, A107, 2016 | 521 | 2016 |
| Planck 2013 results. I. Overview of products and scientific results P Collaboration, PAR Ade, N Aghanim, MIR Alves, C Armitage-Caplan, ... | 441 | 2013 |
| Planck 2018 results-VII. Isotropy and statistics of the CMB Y Akrami, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, AJ Banday, ... Astronomy & Astrophysics 641, A7, 2020 | 259 | 2020 |
| Planck intermediate results-XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies N Aghanim, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 596, A109, 2016 | 228 | 2016 |
| Planck 2018 results-XI. Polarized dust foregrounds Y Akrami, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, AJ Banday, ... Astronomy & Astrophysics 641, A11, 2020 | 189 | 2020 |
| Power asymmetry in WMAP and Planck temperature sky maps as measured by a local variance estimator Y Akrami, Y Fantaye, A Shafieloo, HK Eriksen, FK Hansen, AJ Banday, ... The Astrophysical Journal Letters 784 (2), L42, 2014 | 186 | 2014 |
| Planck 2018 results-XII. Galactic astrophysics using polarized dust emission N Aghanim, Y Akrami, MIR Alves, M Ashdown, J Aumont, C Baccigalupi, ... Astronomy & Astrophysics 641, A12, 2020 | 170 | 2020 |
| No evidence for extensions to the standard cosmological model A Heavens, Y Fantaye, E Sellentin, H Eggers, Z Hosenie, S Kroon, ... Physical review letters 119 (10), 101301, 2017 | 154 | 2017 |
| Planck intermediate results-LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters N Aghanim, Y Akrami, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astronomy & Astrophysics 607, A95, 2017 | 150 | 2017 |
| Planck results. III. High Frequency Instrument data processing and frequency maps N Aghanim, Y Akrami, M Ashdown, J Aumont, C Baccigalupi, M Ballardini, ... Astron. Astrophys., A (), arXiv:.[astro-ph. CO], 2020 | 117 | 2020 |
Domenico MarinucciDepartment of Mathematics, University of Rome Tor VergataAdresse e-mail validée de mat.uniroma2.it
