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Disambiguation of "Fialkov, Anastasia"

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Strong 21-cm fluctuations and anisotropy due to the line-of-sight effect of radio galaxies at cosmic dawn

, , , and . (2023)cite arxiv:2301.04585Comment: Submitted to MNRAS.

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Anastasia Schneider

Einfluss von probiotischen Bakterien auf die Signalgebung dendritischer Zellen. Uni München, (2009)

Anastasia Lange

Anastasia Loman

Anastasia Noglik

Anastasia Bahr

 

Other publications of authors with the same name

Marginal Bayesian Statistics Using Masked Autoregressive Flows and Kernel Density Estimators with Examples in Cosmology, , , , , and . (2022)cite arxiv:2207.11457Comment: Accepted for presentation at MaxEnt22.21cmVAE: A VAE-based Emulator of the 21-cm Global Signal, , and . (2021)cite arxiv:2107.05581Comment: 10 pages, 5 figures, 2 tables (including appendices). Submitted to ApJ.First star-forming structures in fuzzy cosmic filaments, , , , , , , , , and 3 other author(s). (2019)cite arxiv:1910.01653Comment: 6 pages, 2 figures, accepted to Phys. Rev. Lett.Extracting the Global Signal from 21-cm Fluctuations: the Multi-Tracer Approach, , and . (2019)cite arxiv:1904.10857Comment: 12 pages, 9 figures, submitted to MNRAS.Machine Learning to Decipher the Astrophysical Processes at Cosmic Dawn, , , and . (2022)cite arxiv:2201.08205Comment: Submitted to MNRAS on January 19th.A Fast Radio Burst Occurs Every Second throughout the Observable Universe, and . (Aug 29, 2017)Peering into the Dark (Ages) with Low-Frequency Space Interferometers, , , , , , , , , and 21 other author(s). (2019)cite arxiv:1908.04296Comment: 24 pages, 8 figures, 3 tables; White paper submitted to ESA Voyage 2050.Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies, , , , , , , , , and 4 other author(s). (2019)cite arxiv:1911.05746Comment: 19 pages, 12 figures, submitted to MNRAS.Bayesian Data Analysis for Sky-averaged 21-cm Experiments in the Presence of Ionospheric Effects, , , and . (2022)cite arxiv:2204.10859Comment: 8 pages, 7 figures, 7 tables.The subtlety of Ly-a photons: changing the expected range of the 21-cm signal, , and . (2021)cite arxiv:2101.01777.