activity
20132024
most citedCosmological neutrino simulations at extreme scale

60 citations · 607 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.CO2024★ 1 cited

Systematic analysis of Parity-Violating modes

Hong-Ming Zhu, Ue-Li Pen

Recent reports of cosmological parity violation in the 4PCF raises the question of how such violations could be systematically generated. Here we present a constructive procedure t…

astro-ph.CO2022

Cosmic tidal reconstruction in redshift space

Shi-Hui Zang, Hong-Ming Zhu, Marcel Schmittfull +1

The gravitational coupling between large- and small-scale density perturbations leads to anisotropic distortions to the local small-scale matter fluctuations. Such local anisotropi…

astro-ph.CO2022★ 6 cited

Galaxy Spin Classification I: Z-wise vs S-wise Spirals With Chirality Equivariant Residual Network

He Jia, Hong-Ming Zhu, Ue-Li Pen

The angular momentum of galaxies (galaxy spin) contains rich information about the initial condition of the Universe, yet it is challenging to efficiently measure the spin directio…

astro-ph.IM2022★ 60 cited

BURSTT: Bustling Universe Radio Survey Telescope in Taiwan

Hsiu-Hsien Lin, Kai-yang Lin, Chao-Te Li +44

Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1,000 times per day, all-sky, for a fluence threshold 5 Jy ms at 600 MHz. The FRB radio-…

astro-ph.CO2022★ 14 cited

Extracting high-order cosmological information in galaxy surveys with power spectra

Yuting Wang, Gong-Bo Zhao, Kazuya Koyama +11

The reconstruction method was proposed more than a decade ago to boost the signal of baryonic acoustic oscillations measured in galaxy redshift surveys, which is one of key probes…

astro-ph.CO2021★ 6 cited

Cosmic Tidal Reconstruction with Halo Fields

Hong-Ming Zhu, Tian-Xiang Mao, Ue-Li Pen

The gravitational coupling between large-scale perturbations and small-scale perturbations leads to anisotropic distortions of the small-scale matter distribution. The measured loc…

astro-ph.CO2021★ 12 cited

Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure

Yuhao Li, Hong-Ming Zhu, Baojiu Li

Potential features in the primordial power spectrum have been searched for in galaxy surveys in recent years since these features can assist in understanding the nature of inflatio…

astro-ph.CO2020★ 1 cited

Cosmic microwave background lensing with optimal convergence and shear estimators

Hong-Ming Zhu, Ue-Li Pen

We present the optimal convergence and shear estimators for lensing reconstruction from the cosmic microwave background temperature field. This generalizes the deflection estimator…

astro-ph.CO2020★ 34 cited

Quantifying the Line-of-Sight Halo Contribution to the Dark Matter Convergence Power Spectrum from Strong Gravitational Lenses

Atınç Çağan Şengül, Arthur Tsang, Ana Diaz Rivero +3

Galaxy-galaxy strong gravitational lenses have become a popular probe of dark matter (DM) by providing a window into structure formation on the smallest scales. In particular, the…

astro-ph.CO2019★ 10 cited

Reconstruction with velocities

Hong-Ming Zhu, Martin White, Simone Ferraro +1

Reconstruction is becoming a crucial procedure of galaxy clustering analysis for future spectroscopic redshift surveys to obtain subpercent level measurement of the baryon acoustic…

astro-ph.CO2019★ 9 cited

Nonlinear Reconstruction of the Velocity Field

Yu Yu, Hong-Ming Zhu

We propose a new velocity reconstruction method based on the displacement estimation by recently developed methods. The velocity is first reconstructed by transfer functions in Lag…

astro-ph.CO2019★ 12 cited

Measuring dark matter-neutrino relative velocity on cosmological scales

Hong-Ming Zhu, Emanuele Castorina

We present a new method to measure neutrino masses using the dark matter-neutrino relative velocity. The relative motion between dark matter and neutrinos results in a parity-odd b…

astro-ph.CO2019★ 12 cited

Inflation and Dark Energy from spectroscopy at

Simone Ferraro, Michael J. Wilson, Muntazir Abidi +140

The expansion of the Universe is understood to have accelerated during two epochs: in its very first moments during a period of Inflation and much more recently, at , when D…

astro-ph.CO2018★ 18 cited

The Cross-correlation of KSZ Effect and 21 cm Intensity Mapping with Tidal Reconstruction

Dongzi Li, Hong-Ming Zhu, Ue-Li Pen

We discuss the possibility of studying diffuse baryon distributions with kinematic Sunyaev-Zel'dovich (kSZ) effect by correlating cosmic microwave background (CMB) temperature fluc…

astro-ph.CO2017★ 26 cited

Nonlinear reconstruction of redshift space distortions

Hong-Ming Zhu, Yu Yu, Ue-Li Pen

We apply nonlinear reconstruction to the dark matter density field in redshift space and solve for the nonlinear mapping from the initial Lagrangian position to the final redshift…

astro-ph.CO2017★ 36 cited

Isobaric Reconstruction of the Baryonic Acoustic Oscillation

Xin Wang, Hao-Ran Yu, Hong-Ming Zhu +3

In this paper, we report a significant recovery of the linear baryonic acoustic oscillation (BAO) signature by applying the isobaric reconstruction algorithm to the non-linear matt…

astro-ph.CO2017★ 32 cited

Halo nonlinear reconstruction

Yu Yu, Hong-Ming Zhu, Ue-Li Pen

We apply the nonlinear reconstruction method to simulated halo fields. For halo number density at , corresponding to the SDSS ma…

astro-ph.CO2016★ 43 cited

Nonlinear reconstruction

Hong-Ming Zhu, Yu Yu, Ue-Li Pen +2

We present a direct approach to nonparametrically reconstruct the linear density field from an observed nonlinear map. We solve for the unique displacement potential consistent wit…

astro-ph.CO2016★ 60 cited

Cosmological neutrino simulations at extreme scale

J. D. Emberson, Hao-Ran Yu, Derek Inman +8

Constraining neutrino mass remains an elusive challenge in modern physics. Precision measurements are expected from several upcoming cosmological probes of large-scale structure. A…

astro-ph.CO2016★ 34 cited

Measurement of the Cold Dark Matter-Neutrino Dipole in the TianNu Simulation

Derek Inman, Hao-Ran Yu, Hong-Ming Zhu +6

Measurements of neutrino mass in cosmological observations rely on two point statistics that are hindered by significant degeneracies with the optical depth and galaxy bias. The re…

astro-ph.CO2016★ 12 cited

Nonlinear -mode clustering in Lagrangian space

Hao-Ran Yu, Ue-Li Pen, Hong-Ming Zhu

We study the nonlinear -mode clustering in Lagrangian space by using large scale structure -body simulations and use the displacement field information in Lagrangian space to…

astro-ph.CO2016★ 30 cited

Recovering lost 21 cm radial modes via cosmic tidal reconstruction

Hong-Ming Zhu, Ue-Li Pen, Yu Yu +1

21 cm intensity mapping has emerged as a promising technique to map the large-scale structure of the Universe, at redshifts from 1 to 10. Unfortunately, many of the key cross-c…

astro-ph.CO2016★ 39 cited

Differential Neutrino Condensation onto Cosmic Structure

Hao-Ran Yu, J. D. Emberson, Derek Inman +12

Astrophysical techniques have pioneered the discovery of neutrino mass properties. Current cosmological observations give an upper bound on neutrino masses by attempting to disenta…

astro-ph.CO2016★ 9 cited

Primordial density and BAO reconstruction

Hong-Ming Zhu, Ue-Li Pen, Xuelei Chen

We present a new method to reconstruct the primordial (linear) density field using the estimated nonlinear displacement field. The divergence of the displacement field gives the re…