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Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update

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arxiv 1702.03272 v1 pith:UGKXLCC5 submitted 2017-02-10 astro-ph.CO

Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update

classification astro-ph.CO
keywords cosmologicalconstraintsdataanalysiscosmologydifferenceslambdaneutrino
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We present cosmological constraints from the combination of the full mission 9-year WMAP release and small-scale temperature data from the pre-Planck ACT and SPT generation of instruments. This is an update of the analysis presented in Calabrese et al. 2013 and highlights the impact on $\Lambda$CDM cosmology of a 0.06 eV massive neutrino - which was assumed in the Planck analysis but not in the ACT/SPT analyses - and a Planck-cleaned measurement of the optical depth to reionization. We show that cosmological constraints are now strong enough that small differences in assumptions about reionization and neutrino mass give systematic differences which are clearly detectable in the data. We recommend that these updated results be used when comparing cosmological constraints from WMAP, ACT and SPT with other surveys or with current and future full-mission Planck cosmology. Cosmological parameter chains are publicly available on the NASA's LAMBDA data archive.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth

    astro-ph.CO 2023-04 accept novelty 6.0

    ACT DR6 yields a 2.3% precise CMB lensing power spectrum with A_lens = 1.013 ± 0.023 relative to Planck 2018 Lambda CDM, giving S8 = 0.818 ± 0.022 and no evidence for suppressed structure growth.