output
20022025
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2016Show all

175 papers · 1 filter

astro-ph.GA2016155 cited

CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field

H. Nayyeri, S. Hemmati, B. Mobasher +36

We present a multi-wavelength photometric catalog in the COSMOS field as part of the observations by the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). T…

cond-mat.stat-mech20165 cited

Effect of film thickness on the width of percolation threshold in metal-dielectric composites

M. Mokhtari, L. Zekri, A. Kaiss +1

The effect of thickness on the width of the percolation threshold in metal-dielectric composite films was examined. The distribution of current intensities through cubic networks o…

hep-ex201666 cited

Measurement of the CKM angle from a combination of LHCb results

LHCb collaboration, R. Aaij, B. Adeva +765

A combination of measurements sensitive to the CKM angle from LHCb is performed. The inputs are from analyses of time-integrated , $B^{0} \rightarrow D K…

astro-ph.GA2016

Dynamical modelling of galactic disc outskirts

E. Athanassoula

I review briefly some dynamical models of structures in the outer parts of disc galaxies, including models of polar rings, tidal tails and bridges. I then discuss the density distr…

astro-ph.GA201656 cited

Metallicity-dependendent kinematics and morphology of the Milky Way bulge

E. Athanassoula, S. A. Rodionov, N. Prantzos

We use N-body chemo-dynamic simulations to study the coupling between morphology, kinematics and metallicity of the bar/bulge region of our Galaxy. We make qualitative comparisons…

astro-ph.CO201636 cited

A Type II Supernova Hubble diagram from the CSP-I, SDSS-II, and SNLS surveys

T. de Jaeger, S. González-Gaitán, M. Hamuy +15

The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in…