output
20022013
most citedDoping graphene with metal contacts

2.6k citations

Showing 2013 · astro-ph.COShow all

5 papers · 2 filters

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.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…

astro-ph.CO201362 cited

A Herschel Survey of the [N II] 205 micron Line in Local Luminous Infrared Galaxies --- The [N II] 205 micron Emission as a Star Formation Rate Indicator

Yinghe Zhao, Nanyao Lu, C. Kevin Xu +16

We present, for the first time, a statistical study of [N II] 205 mciron line emission for a large sample of local luminous infrared galaxies using Herschel Spectral and Photometri…

astro-ph.CO20139 cited

Probing the nature of compact ultra-steep spectrum radio sources with the e-EVN and e-MERLIN

Megan K. Argo, Zsolt Paragi, Huub Röttgering +3

We present first results from electronic Multi-Element Remotely Linked Interferometer Network (e-MERLIN) and electronic European VLBI Network (e-EVN) observations of a small sample…

astro-ph.CO201340 cited

Deep, wide-field, global VLBI observations of the Hubble Deep Field North and Flanking Fields

S. Chi, P. D. Barthel, M. A. Garrett

Dust is commonly present in weakly radio emitting star-forming galaxies and this dust may obscure the signatures of accreting black holes in these objects. We aim to uncover weak a…