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Cosmological imprints in the filament with DisPerSE
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Galaxy Superclusters and Their Complexes in the Cosmic Web
THE THREE HUNDRED project: Estimating the dependence of gas filaments on the mass of galaxy clusters
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Evolution of cosmic filaments in the MTNG simulation
Daniela Galárraga-Espinosa, Corentin Cadiou, Céline Gouin, Simon D. M. White, Volker Springel, Rüdiger Pakmor, Boryana Hadzhiyska, Sownak Bose, Fulvio Ferlito, Lars Hernquist, Rahul Kannan, Monica Barrera, Ana Maria Delgado and César Hernández-Aguayo Astronomy & Astrophysics 684 A63 (2024) https://doi.org/10.1051/0004-6361/202347982
Estimating the Masses of Supercluster-scale Filaments from Redshift Dispersions
Large-scale structure around the Fornax-Eridanus complex
M. A. Raj, P. Awad, R. F. Peletier, R. Smith, U. Kuchner, R. van de Weygaert, N. I. Libeskind, M. Canducci, P. Tiňo and K. Bunte Astronomy & Astrophysics 690 A92 (2024) https://doi.org/10.1051/0004-6361/202450815
Hierarchical reconstruction of the cosmic web, the H-Spine method
The environmental dependence of the stellar mass–gas metallicity relation in Horizon Run 5
Aaron R Rowntree, Ankit Singh, Fiorenzo Vincenzo, Brad K Gibson, Céline Gouin, Daniela Galárraga-Espinosa, Jaehyun Lee, Juhan Kim, Clotilde Laigle, Changbom Park, Christophe Pichon, Gareth Few, Sungwook E Hong and Yonghwi Kim Monthly Notices of the Royal Astronomical Society 531(4) 3858 (2024) https://doi.org/10.1093/mnras/stae1384
Tracing gaseous filaments connected to galaxy clusters: The case study of Abell 2744
Testing Lyα Emitters and Lyman-break Galaxies as Tracers of Large-scale Structures at High Redshifts
Sang Hyeok Im, Ho Seong Hwang, Jaehong Park, Jaehyun Lee, Hyunmi Song, Stephen Appleby, Yohan Dubois, C. Gareth Few, Brad K. Gibson, Juhan Kim, Yonghwi Kim, Changbom Park, Christophe Pichon, Jihye Shin, Owain N. Snaith, M. Celeste Artale, Eric Gawiser, Lucia Guaita, Woong-Seob Jeong, Kyoung-Soo Lee, Nelson Padilla, Vandana Ramakrishnan, Paulina Troncoso and Yujin Yang The Astrophysical Journal 972(2) 196 (2024) https://doi.org/10.3847/1538-4357/ad67d2
Statistical properties of filaments in the cosmic web
Youcai Zhang, Hong Guo, Xiaohu Yang and Peng Wang Monthly Notices of the Royal Astronomical Society 533(1) 1048 (2024) https://doi.org/10.1093/mnras/stae1914
Towards unbiased recovery of cosmic filament properties: the role of spine curvature and optimized smoothing
Filaments of the Slime Mold Cosmic Web and How They Affect Galaxy Evolution
Farhanul Hasan, Joseph N. Burchett, Douglas Hellinger, Oskar Elek, Daisuke Nagai, S. M. Faber, Joel R. Primack, David C. Koo, Nir Mandelker and Joanna Woo The Astrophysical Journal 970(2) 177 (2024) https://doi.org/10.3847/1538-4357/ad4ee2
Mary Crone Odekon, Michael G. Jones, Lucas Graham, Jessica Kelley-Derzon and Evan Halstead The Astrophysical Journal 935(2) 130 (2022) https://doi.org/10.3847/1538-4357/ac815b
Anisotropic satellite accretion on to the Local Group with HESTIA
Alexandra Dupuy, Noam I Libeskind, Yehuda Hoffman, et al. Monthly Notices of the Royal Astronomical Society 516(3) 4576 (2022) https://doi.org/10.1093/mnras/stac2486
Gas distribution from clusters to filaments in IllustrisTNG
Regularization of Mixture Models for Robust Principal Graph Learning
Tony Bonnaire, Aurelien Decelle and Nabila Aghanim IEEE Transactions on Pattern Analysis and Machine Intelligence 44(12) 9119 (2022) https://doi.org/10.1109/TPAMI.2021.3124973
Properties of gas phases around cosmic filaments atz= 0 in the IllustrisTNG simulation
The Four Cosmic Tidal Web Elements from the β-skeleton
John F. Suárez-Pérez, Yeimy Camargo, Xiao-Dong Li and Jaime E. Forero-Romero The Astrophysical Journal 922(2) 204 (2021) https://doi.org/10.3847/1538-4357/ac1fed
Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects
Detection and analysis of cluster–cluster filaments
Luis A Pereyra, Mario A Sgró, Manuel E Merchán, Federico A Stasyszyn and Dante J Paz Monthly Notices of the Royal Astronomical Society 499(4) 4876 (2020) https://doi.org/10.1093/mnras/staa3112
Populations of filaments from the distribution of galaxies in numerical simulations