Virgo Filaments II: Catalog and First Results on the Effect of Filaments on galaxy properties
G. Castignani, B. Vulcani, R. A. Finn, F. Combes, P. Jablonka, G., Rudnick, D. Zaritsky, K. Whalen, K. Conger, G. De Lucia, V. Desai, R. A., Koopmann, J. Moustakas, D. J. Norman, and M. Townsend

TL;DR
This paper constructs a detailed galaxy catalog around the Virgo cluster, identifying 13 filaments and analyzing how filament environments influence galaxy properties and evolution.
Contribution
It provides the first comprehensive catalog of galaxies and filament structures around Virgo, revealing environmental effects on galaxy morphology and density.
Findings
13 filaments identified around Virgo, spanning several Mpc
Filaments are thin, low-density, and transitional environments
Denser filaments have higher fractions of early-type galaxies
Abstract
Virgo is the nearest galaxy cluster; it is thus ideal for studies of galaxy evolution in dense environments in the local Universe. It is embedded in a complex filamentary network of galaxies and groups, which represents the skeleton of the large scale Laniakea supercluster. Here we assemble a comprehensive catalog of galaxies extending up to ~12 virial radii in projection from Virgo to revisit the Cosmic Web structure around it. This work is the foundation of a series of papers that will investigate the multi-wavelength properties of galaxies in the Cosmic Web around Virgo. We match spectroscopically confirmed sources from several databases and surveys including HyperLeda, NASA Sloan Atlas, NED, and ALFALFA. The sample consists of ~7000 galaxies. By exploiting a tomographic approach, we identify 13 filaments, spanning several Mpc in length. Long > 17 Mpc/h filaments, tend to be thin (<…
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