output
19922026
most citedElectric Field Effect in Atomically Thin Carbon Films

66.7k citations

Showing 2014Show all

525 papers · 1 filter

astro-ph.HE2014★ 26 cited

Testing Gravity with Pulsars in the SKA Era

Lijing Shao, Ingrid H. Stairs, John Antoniadis +12

The Square Kilometre Array (SKA) will use pulsars to enable precise measurements of strong gravity effects in pulsar systems, which yield tests of gravitational theories that canno…

astro-ph.IM2014★ 11 cited

A Cosmic Census of Radio Pulsars with the SKA

E. F. Keane, B. Bhattacharyya, M. Kramer +16

The Square Kilometre Array (SKA) will make ground breaking discoveries in pulsar science. In this chapter we outline the SKA surveys for new pulsars, as well as how we will perform…

astro-ph.HE2014★ 159 cited

Discovery of PSR J1227-4853: A transition from a low-mass X-ray binary to a redback millisecond pulsar

Jayanta Roy, Paul S. Ray, Bhaswati Bhattacharyya +12

XSS J12270-4859 is an X-ray binary associated with the Fermi LAT gamma-ray source 1FGL J1227.9-4852. In 2012 December, this source underwent a transition where the X-ray and optica…

cond-mat.mes-hall2014★ 1.7k cited

Light-emitting diodes by bandstructure engineering in van der Waals heterostructures

F. Withers, O. Del Pozo-Zamudio, A. Mishchenko +8

The advent of graphene and related 2D materials has recently led to a new technology: heterostructures based on these atomically thin crystals. The paradigm proved itself extremely…

cond-mat.mes-hall2014★ 776 cited

Square ice in graphene nanocapillaries

G. Algara-Siller, O. Lehtinen, F. C. Wang +5

Adsorbed layers of water are ubiquitously present at surfaces and fill in microscopic pores, playing a central role in many phenomena in such diverse fields as materials science, g…

astro-ph.GA2014★ 12 cited

The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83

A. G. Jones, G. J. Bendo, M. Baes +13

We examine the relation between polycyclic aromatic hydrocarbon (PAH) emission at 8 microns and far-infrared emission from hot dust grains at 24 microns and from large dust grains…