activity
20112018
most citedEnhanced global signal of neutral hydrogen due to excess radiation at cosmic dawn

247 citations · 415 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2018★ 247 cited

Enhanced global signal of neutral hydrogen due to excess radiation at cosmic dawn

Chang Feng, Gilbert Holder

We revisit the global 21cm signal calculation incorporating a possible radio background at early times, and find that the global 21cm signal shows a much stronger absorption featur…

astro-ph.CO2018★ 6 cited

Detecting Electron Density Fluctuations from Cosmic Microwave Background Polarization using a Bispectrum Approach

Chang Feng, Gilbert Holder

Recent progress in high sensitivity Cosmic Microwave Background (CMB) polarization experiments opens up a window on large scale structure (LSS), as CMB polarization fluctuations on…

astro-ph.CO2017★ 31 cited

Current and Future Constraints on Primordial Magnetic Fields

Dylan R. Sutton, Chang Feng, Christian L. Reichardt

We present new limits on the amplitude of potential primordial magnetic fields (PMFs) using temperature and polarization measurements of the cosmic microwave background (CMB) from…

astro-ph.CO2017★ 22 cited

A Halo Model Approach to the and Cross-correlation

Chang Feng, Asantha Cooray, Brian Keating

We present a halo-model-based approach to calculate the cross-correlation between HI intensity fluctuations and emitters (LAE) during the epoch of reioniza…

astro-ph.CO2016★ 39 cited

Probing the Intergalactic Medium with Ly and 21 cm Fluctuations

Caroline Heneka, Asantha Cooray, Chang Feng

We study 21cm and Ly fluctuations, as well as H, while distinguishing between Ly emission of galactic, diffuse, and scattered intergalactic medium (IG…

astro-ph.CO2016★ 18 cited

Planck Lensing and Cosmic Infrared Background Cross-Correlation with Fermi-LAT: Tracing Dark Matter Signals in the Gamma-Ray Background

Chang Feng, Asantha Cooray, Brian Keating

The extragalactic -ray background and its spatial anisotropy could potentially contain a signature of dark matter (DM) annihilation or particle decay. Astrophysical foregrounds,…

astro-ph.IM2015★ 40 cited

Modeling atmospheric emission for CMB ground-based observations

J. Errard, P. A. R. Ade, Y. Akiba +72

Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies t…

astro-ph.CO2011★ 12 cited

Reconstruction of Gravitational Lensing Using WMAP 7-Year Data

Chang Feng, Brian Keating, Hans P. Paar +1

Gravitational lensing by large scale structure introduces non-Gaussianity into the Cosmic Microwave Background and imprints a new observable, which can be used as a cosmological pr…