activity
20072022
most citedA Chandra Study of Temperature Substructures in Intermediate-Redshift Galaxy Clusters

26 citations · 55 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2022

Global CD/EoR Signal Detection with a Dense Digital Beamforming Array and Beyond

Junhua Gu, Jingying Wang, Huanyuan Shan +5

The global neutral hydrogen 21 cm signal extracted from the all-sky averaged radio spectra is one of the signatures of the Cosmic Dawn and Epoch of Reionization (CD/EoR). The frequ…

astro-ph.CO2020

HI intensity mapping with MeerKAT: Calibration pipeline for multi-dish autocorrelation observations

Jingying Wang, Mario G. Santos, Philip Bull +10

While most purpose-built 21cm intensity mapping experiments are close-packed interferometer arrays, general-purpose dish arrays should also be capable of measuring the cosmological…

astro-ph.CO2020

HI intensity mapping with MeerKAT: 1/f noise analysis

Yichao Li, Mario G. Santos, Keith Grainge +2

The nature of the time correlated noise component (the 1/f noise) of single dish radio telescopes is critical to the detectability of the HI signal in intensity mapping experiments…

astro-ph.CO20206 cited

Direct Parameter Inference from Global EoR Signal with Bayesian Statistics

Junhua Gu, Jingying Wang

In the observation of sky-averaged HI signal from Epoch of Reionization, model parameter inference can be a computation-intensive work, which makes it hard to perform a direct one-…

astro-ph.CO201911 cited

Contribution of Radio Halos to the Foreground for SKA EoR Experiments

Weitian Li, Haiguang Xu, Zhixian Ma +11

The overwhelming foreground contamination is one of the primary impediments to probing the Epoch of Reionization (EoR) through measuring the redshifted 21 cm signal. Among various…

astro-ph.GA20198 cited

Revealing A Head-on Major Merger in the Nearby NGC 6338 Group with Chandra and VLA observations

Yu Wang, Fuyao Lui, Zhiqiang Shen +3

By analyzing the Chandra archival data of the nearby NGC 6338 galaxy group, we identify two X-ray bright clumps (N-clump and S-clump) within the central 100 kpc, and detect an arc-…