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Velocity waves in the Hubble diagram: signature of local galaxy clusters

, , , , and . (2023)cite arxiv:2301.01305Comment: re-submitted to MNRAS on November the 8th 2022, 10 pages, 8 figures and 2 tables.

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On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin, , , , and . (2021)cite arxiv:2109.14623Comment: 24 pages, 21 figures, under review at A&A, comments welcome.Cascade of Phase Transitions for Multi-Scale Clustering., , and . CoRR, (2020)Regularization of Mixture Models for Robust Principal Graph Learning., , and . CoRR, (2021)Regularization of Mixture Models for Robust Principal Graph Learning., , and . IEEE Trans. Pattern Anal. Mach. Intell., 44 (12): 9119-9130 (2022)Predicting large scale cosmological structure evolution with GAN-based autoencoders., , , and . CoRR, (2024)Encoding large scale cosmological structure with Generative Adversarial Networks., , and . CoRR, (2020)Cosmological Non-Gaussian Signature Detection: Comparing Performance of Different Statistical Tests., , , , and . EURASIP J. Adv. Signal Process., 2005 (15): 2470-2485 (2005)Adapted Method for Separating Kinetic SZ Signal from Primary CMB Fluctuations., and . EURASIP J. Adv. Signal Process., 2005 (15): 2413-2425 (2005)Velocity waves in the Hubble diagram: signature of local galaxy clusters, , , , and . (2023)cite arxiv:2301.01305Comment: re-submitted to MNRAS on November the 8th 2022, 10 pages, 8 figures and 2 tables.