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The Astropy Problem, , , , , , , , , и 144 other автор(ы). eprint arXiv:astro-ph.IM/1610.03159, (октября 2016)The Atacama Cosmology Telescope: Detection of Patchy Screening of the Cosmic Microwave Background, , , , , , , , , и 30 other автор(ы). (2024)Constraining CMB temperature evolution with Sunyaev-Zel'dovich galaxy clusters from the Atacama Cosmology Telescope, , , , , , , , , и 22 other автор(ы). (2021)cite arxiv:2106.12467.The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy, , , , , , , , , и 32 other автор(ы). (2021)cite arxiv:2109.04451Comment: 25+20 pages, 6+18 figures, submitted to PRD.The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access, , , , , , , , , и 39 other автор(ы). (2021)cite arxiv:2103.03154Comment: 21 pages, 8 figures. Data and notebooks available on LAMBDA https://lambda.gsfc.nasa.gov/product/act/.The Atacama Cosmology Telescope: High-resolution component-separated maps across one-third of the sky, , , , , , , , , и 144 other автор(ы). (2023)cite arxiv:2307.01258Comment: The Compton-y map and associated products will be made publicly available upon publication of the paper. The CMB T and E mode maps will be made available when the DR6 maps are made public.The Atacama Cosmology Telescope: Probing the Baryon Content of SDSS DR15 Galaxies with the Thermal and Kinematic Sunyaev-Zel'dovich Effects, , , , , , , , , и 40 other автор(ы). (2021)cite arxiv:2101.08373Comment: 19 pages, 9 figures.The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies, , , , , , , , , и 40 other автор(ы). (2021)cite arxiv:2101.08374Comment: 16 pages, 9 figures.The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth, , , , , , , , , и 148 other автор(ы). (2023)cite arxiv:2304.05202Comment: 45+21 pages, 50 figures. Prepared for submission to ApJ. Also see companion papers Madhavacheril et al and MacCrann et al.The abundance of ultra-diffuse galaxies from groups to clusters: UDGs are relatively more common in more massive haloes, , , , , , , , , и 10 other автор(ы). (2017)cite arxiv:1706.02704Comment: 11 pages, 8 figures. Submitted for publication in A&A.