output
20022011
most citedDoping graphene with metal contacts

2.6k citations

Showing 2011 · astro-ph.COShow all

7 papers · 2 filters

astro-ph.CO20111.5k cited

A luminous quasar at a redshift of z = 7.085

Daniel J. Mortlock, Stephen J. Warren, Bram P. Venemans +14

The intergalactic medium was not completely reionized until approximately a billion years after the Big Bang, as revealed by observations of quasars with redshifts of less than 6.5…

astro-ph.CO201182 cited

Morphological evolution of galaxies from ultradeep HST WFC3 imaging: the Hubble sequence at z~2

Daniel Szomoru, Marijn Franx, Rychard J. Bouwens +4

We use ultradeep HST WFC3/IR imaging of the HUDF to investigate the rest-frame optical morphologies of a mass-selected sample of galaxies at z~2. We find a large variety of galaxy…

astro-ph.CO2011107 cited

The stellar velocity dispersion of a compact massive galaxy at z=1.80 using X-Shooter: confirmation of the evolution in the mass-size and mass-dispersion relations

Jesse van de Sande, Mariska Kriek, Marijn Franx +7

Recent photometric studies have shown that early-type galaxies at fixed stellar mass were smaller and denser at earlier times. In this paper we assess that finding by deriving the…

astro-ph.CO201187 cited

Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS

Ivan Valtchanov, J. Virdee, R. J. Ivison +51

We present Herschel-SPIRE Fourier Transform Spectrometer (FTS) and radio follow-up observations of two Herschel-ATLAS (H-ATLAS) detected strongly lensed distant galaxies. In one of…

astro-ph.CO201132 cited

Mass, Light and Colour of the Cosmic Web in the Supercluster SCL2243-0935 (z=0.447)

Mischa Schirmer, Hendrik Hildebrandt, Konrad Kuijken +1

Context: In 2.2m MPG-ESO/WFI data we discovered several mass peaks through weak lensing, forming a possible supercluster at redshift 0.45. Through multi-colour wide-field imaging w…

astro-ph.CO20119 cited

A new perspective on the submillimetre galaxy MM 18423+5938 at redshift 3.9296 from radio continuum imaging

J. P. McKean, A. Berciano Alba, F. Volino +5

The bright submillimetre (sub-mm) galaxy MM 18423+5938 at redshift 3.9296 has been predicted from mid-infrared and millimetre photometry to have an exceptionally large total infrar…