activity
20002022
most citedEnabling III-V-based optoelectronics with low-cost dynamic hydride vapor phase epitaxy

62 citations · 75 across the 7 of their papers we have counts for

collaborators

7 papers

cond-mat.mtrl-sci2022

Consideration of the Intricacies Inherent in Molecular Beam Epitaxy of the NaCl/GaAs System

Brelon J. May, Jae Jin Kim, Patrick Walker +4

The high cost of substrates for III-V growth can be cost limiting for technologies that require large semiconductor areas. Thus, being able to separate device layers and reuse the…

physics.app-ph2021★ 4 cited

Surface chemistry models for GaAs epitaxial growth and hydride cracking using reacting flow simulations

Malik Hassanaly, Hariswaran Sitaraman, Kevin L. Schulte +5

Hydride Vapor Phase Epitaxy (HVPE) is a promising technology that can aid in the cost reduction of III-V materials and devices manufacturing, particularly high-efficiency solar cel…

physics.app-ph2018★ 62 cited

Enabling III-V-based optoelectronics with low-cost dynamic hydride vapor phase epitaxy

John Simon, Kevin L. Schulte, Kelsey Horowitz +3

Silicon is the dominant semiconductor in many semiconductor device applications for a variety of reasons, including both performance and cost. III-V materials have improved perform…

astro-ph2008

Wide Area X-ray Surveys for AGN and Starburst Galaxies

A. Ptak

While often the point sources in X-ray surveys are dominated by AGN, with the high sensitivity of modern X-ray telescopes such as Chandra and XMM-Newton normal/starburst galaxies a…

astro-ph2007★ 1 cited

X-ray Luminosity Functions of Normal Galaxies in the GOODS

A. Ptak, B. Mobasher, A. Hornschemeier +2

We present soft (0.5-2 keV) X-ray luminosity functions (XLFs) in the Great Observatories Origins Deep Survey (GOODS) fields, derived for galaxies at z~0.25 and 0.75. SED fitting wa…

astro-ph2001

Resolving the X-ray Spectral Paradox: XMM-Newton Spectra of Faint Sources in the Lockman Hole

R. E. Griffiths, A. Ptak, T. Miyaji

Using 100ks of XMM-Newton data on the Lockman Hole, we show how the X-ray background 'spectral paradox' is being resolved. We find the summed spectra of the Type I AGN, Type II AGN…