activity
20162020
most citedGenerating Log-normal Mock Catalog of Galaxies in Redshift Space

63 citations · 78 across the 2 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2020

A-priori Validation of Subgrid-scale Models for Astrophysical Turbulence

Chia-Yu Hu, Chi-Ting Chiang

We perform a-priori validation tests of subgrid-scale (SGS) models for the turbulent transport of momentum, energy and passive scalars. To this end, we conduct two sets of high-res…

astro-ph.CO2019

Predicting CMB dust foreground using galactic 21 cm data

Guangyu Zhang, Chi-Ting Chiang, Chris Sheehy +2

Understanding large-angular-scale galactic foregrounds is crucial for future CMB experiments aiming to detect -mode polarization from primordial gravitational waves. Traditional…

astro-ph.CO2018

Inferences of in presence of a non-standard recombination

Chi-Ting Chiang, Anže Slosar

Measurements of the Hubble parameter from the distance ladder are in tension with indirect measurements based on the cosmic microwave background (CMB) data and the inverse distance…

astro-ph.CO2018

First detection of scale-dependent linear halo bias in -body simulations with massive neutrinos

Chi-Ting Chiang, Marilena LoVerde, Francisco Villaescusa-Navarro

Using -body simulations with massive neutrino density perturbations, we detect the scale-dependent linear halo bias with high significance. This is the first time that this effe…

astro-ph.CO2018

Probing Decoupling in Dark Sectors with the Cosmic Microwave Background

Gongjun Choi, Chi-Ting Chiang, Marilena LoVerde

The acoustic peaks in the angular power spectrum of cosmic microwave background (CMB) temperature and polarization anisotropies play an important role as a probe of the nature of n…

astro-ph.CO2018

Power spectrum in the presence of large-scale overdensity and tidal fields: breaking azimuthal symmetry

Chi-Ting Chiang, Anže Slosar

We consider the power spectrum of a biased tracer observed in a finite volume in the presence of a large-scale overdensity and tidal fields. Expanding both the observed power spect…