Showing 1–20 of 50 results
/ Date/ Name
Feb 16, 2022Robust sampling for weak lensing and clustering analyses with the Dark Energy SurveyJul 17, 2018Planck 2018 results. XII. Galactic astrophysics using polarized dust emissionJul 17, 2018Planck 2018 results. IV. Diffuse component separationMar 27, 2020Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove IIJul 9, 2020Planck intermediate results. LVII. Joint Planck LFI and HFI data processingMay 11, 2016Planck intermediate results. XLVII. Planck constraints on reionization historyMay 30, 2016Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropiesMay 28, 2021Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sampleMay 14, 2019Planck 2018 results. IX. Constraints on primordial non-GaussianityOct 5, 2018Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak LensingMay 27, 2016Planck intermediate results. XLIX. Parity-violation constraints from polarization dataDec 21, 2016Planck intermediate results. LII. Planet flux densitiesJul 13, 2017Exploring cosmic origins with CORE: mitigation of systematic effectsNov 7, 2025Focus Point on Tensions in Cosmology from Early to Late Universe: Part II: New Directions in the Light of Observations from the Most Modern Astronomical FacilitiesJun 6, 2019Planck 2018 results. VII. Isotropy and Statistics of the CMBJul 30, 2019Planck 2018 results. V. CMB power spectra and likelihoodsJul 17, 2018Planck 2018 results. III. High Frequency Instrument data processing and frequency mapsSep 14, 2020Planck intermediate results. LV. Reliability and thermal properties of high-frequency sources in the Second Planck Catalogue of Compact SourcesJan 15, 2018Planck 2018 results. XI. Polarized dust foregroundsMar 30, 2017Exploring Cosmic Origins with CORE: Cluster Science