# Large Scale Structure in CHILES

## TL;DR

This paper demonstrates the use of DisPerSE to identify cosmic web structures in deepfield galaxy data, analyzing galaxy distributions, their relation to filaments, and the properties of neutral hydrogen across cosmic time.

## Contribution

It introduces a method to identify cosmic web filaments in observational data using DisPerSE and applies it to study galaxy environments and HI properties in the CHILES survey.

## Key findings

- Redder and more massive galaxies are closer to filaments.
- Predicted HI mass fraction varies with distance to filaments.
- Identification of the cosmic web enables future studies of galaxy properties.

## Abstract

We demonstrate that the Discrete Persistent Source Extractor (DisPerSE) can be used with spectroscopic redshifts to define the cosmic web and its distance to galaxies in small area deepfields. Here we analyze the use of DisPerSE to identify structure in observational data. We apply DisPerSE to the distribution of galaxies in the COSMOS field and find the best parameters to identify filaments. We compile a catalog of 11500 spectroscopic redshifts from the Galaxy and Mass Assembly (GAMA) G10 data release. We analyze two-dimensional slices, extract filaments and calculate the distance for each galaxy to its nearest filament. We find that redder and more massive galaxies are closer to filaments. To study the growth of galaxies across cosmic time, and environment, we are carrying out an HI survey covering redshifts z = 0 - 0.45, the COSMOS HI Large Extragalactic Survey (CHILES). In addition we present the predicted HI mass fraction as a function of distance to filaments for the spectroscopically known galaxies in CHILES. Lastly, we discuss the cold gas morphology of a few individual galaxies and their positions with respect to the cosmic web. The identification of the cosmic web, and the ability of CHILES to study the resolved neutral hydrogen morphologies and kinematics of galaxies, will allow future studies of the properties of neutral hydrogen in different cosmic web environments across the redshift range z = 0.1 - 0.45.