output
20022013
most citedDoping graphene with metal contacts

2.6k citations

Showing 2013Show all

25 papers · 1 filter

cond-mat.soft20131 cited

Soliton attenuation and emergent hydrodynamics in fragile matter

N. Upadhyaya, L. R. Gomez, V. Vitelli

Disordered packings of soft grains are fragile mechanical systems that loose rigidity upon lowering the external pressure towards zero. At zero pressure, we find that any infinites…

astro-ph.CO201325 cited

Star Formation Rates in Resolved Galaxies: Calibrations with Near and Far Infrared Data for NGC5055 and NGC6946

Yiming Li, Alison F. Crocker, Daniela Calzetti +21

We use the near--infrared Brγhydrogen recombination line as a reference star formation rate (SFR) indicator to test the validity and establish the calibration of the {\it Herschel}…

astro-ph.EP201315 cited

A sensitivity analysis of the WFCAM Transit Survey for short-period giant planets around M dwarfs

Gábor Kovács, S. Hodgkin, B. Sipőcz +11

The WFCAM Transit Survey (WTS) is a near-infrared transit survey running on the United Kingdom Infrared Telescope (UKIRT), designed to discover planets around M dwarfs. The WTS act…

astro-ph.IM2013161 cited

Calibrating High-Precision Faraday Rotation Measurements for LOFAR and the Next Generation of Low-Frequency Radio Telescopes

C. Sotomayor-Beltran, C. Sobey, J. W. T. Hessels +77

Faraday rotation measurements using the current and next generation of low-frequency radio telescopes will provide a powerful probe of astronomical magnetic fields. However, achiev…

cond-mat.soft20131 cited

Transmission and reflection of strongly nonlinear solitary waves at granular interfaces

A. M. Tichler, L. R. Gomez, N. Upadhyaya +3

The interaction of a solitary wave front with an interface formed by two strongly-nonlinear non-cohesive granular lattices displays rich behaviour, characterized by the breakdown o…

astro-ph.CO201341 cited

The Planetary Nebula Spectrograph survey of S0 galaxy kinematics. Data and Overview

A. Cortesi, M. Arnaboldi, L. Coccato +11

The origins of S0 galaxies remain obscure, with various mechanisms proposed for their formation, likely depending on environment. These mechanisms would imprint different signature…