activity
19962025
most citedAn Efficient Technique to Determine the Power Spectrum from Cosmic Microwave Background Sky Maps

142 citations · 417 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2025

Particle Acceleration in Magnetized Shear-Driven Turbulence

Mingxuan Liu, Mateusz Ruszkowski, Ellen Zweibel +5

Shear flows, ubiquitous in space and astrophysical plasmas, can accelerate particles through turbulence excited by the Kelvin-Helmholtz instability. We present the first numerical…

astro-ph1999★ 67 cited

Observational Signatures of the First Luminous Objects

Siang Peng Oh

The next generation of astronomical instruments will be able to detect dense pockets of ionized gas created by the first luminous objects. The integrated free-free emission from io…

astro-ph1998

Clustering of Ionizing Sources

Siang Peng Oh

Using existing models for the evolution of clustering we show that the first sources are likely to be highly biased and thus strongly clustered. We compute intensity fluctuations f…

astro-ph1998★ 142 cited

An Efficient Technique to Determine the Power Spectrum from Cosmic Microwave Background Sky Maps

Siang Peng Oh, David N. Spergel, Gary Hinshaw

There is enormous potential to advance cosmology from statistical characterizations of cosmic microwave background sky maps. The angular power spectrum of the microwave anisotropy…

astro-ph1997★ 121 cited

Fast Tides in Slow Stars: the Efficiency of Eddy Viscosity

Jeremy Goodman, Siang Peng Oh

The turbulent viscosity of convection is believed to circularize the orbits of close binary stars. When the tidal period is shorter than the turnover time of the largest eddies, tu…

astro-ph1996

Searching for the Kinematical Signature of a Black Hole in M87

David Merritt, Siang Peng Oh

Many theories for the formation of massive black holes in galactic nuclei predict that the stellar motions should be anisotropic within the radius of influence of the black hole. W…