output
20042020
most citedThe Solar Neighborhood XXXV: Distances to 1404 M Dwarf Systems Within 25 pc in the Southern Sky

156 citations

Showing 2016Show all

6 papers · 1 filter

astro-ph.HE20166 cited

Calibrating Column Density Tracers with Gamma-ray Observations of the Ophiuchi Molecular Cloud

Ryan D. Abrahams, Alex Teachey, Timothy A. D. Paglione

Diffuse gamma-ray emission from interstellar clouds results largely from cosmic ray (CR) proton collisions with ambient gas, regardless of the gas state, temperature, or dust prope…

cond-mat.mtrl-sci201633 cited

Field-created diverse quantizations in phosphorenes

Jhao-Ying Wu, Szu-Chao Chen, Godfrey Gumbs

Electronic properties of few-layer phosphorenes are investigated by the generalized tight-binding model. They are greatly diversified by the electric and magnetic fields ( and…

astro-ph.SR2016138 cited

Magnetic Flux Cancellation as the Trigger of Solar Quiet-Region Coronal Jets

Navdeep K. Panesar, Alphonse C. Sterling, Ronald L. Moore +1

We report observations of ten random on-disk solar quiet region coronal jets found in high resolution Extreme Ultraviolet (EUV) images from the Solar Dynamics Observatory (SDO)/Atm…

quant-ph20164 cited

Retrodiction of a sequence of measurement results in qubit interferometers

Mark Hillery, Daniel Koch

We study how well we can retrodict results of measurements made on a quantum system if we can make measurements on its final state. We know what measurements were made, but not the…

cond-mat.mes-hall201614 cited

Effect of Energy Band Gap in Graphene on Negative Refraction through the Veselago Lens and Electron Conductance

Dipendra Dahal, Godfrey Gumbs

A remarkable property of intrinsic graphene is that upon doping, electrons and holes travel through the monolayer thick material with constant velocity which does not depend on ene…

astro-ph.SR201656 cited

Exploring the Role of Sub-micron Sized Dust Grains in the Atmospheres of Red L0 - L6 Dwarfs

Kay Hiranaka, Kelle L. Cruz, Stephanie T. Douglas +2

We examine the hypothesis that the red near-infrared colors of some L dwarfs could be explained by a "dust haze" of small particles in their upper atmospheres. This dust haze would…