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20002022
most citedLight Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

839 citations · 8k across the 72 of their papers we have counts for

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Showing 2015Show all

12 papers · 1 filter

astro-ph.CO2015★ 58 cited

Cross-correlation of gravitational lensing from DES Science Verification data with SPT and Planck lensing

D. Kirk, Y. Omori, A. Benoit-Lévy +89

We measure the cross-correlation between weak lensing of galaxy images and of the cosmic microwave background (CMB). The effects of gravitational lensing on different sources will…

astro-ph.CO2015★ 12 cited

The XMM Cluster Survey: evolution of the velocity dispersion -- temperature relation over half a Hubble time

Susan Wilson, Matt Hilton, Philip J. Rooney +26

We measure the evolution of the velocity dispersion--temperature (--) relation up to using a sample of 38 galaxy clusters drawn from the \textit{XMM}…

astro-ph.CO2015★ 65 cited

Mapping and simulating systematics due to spatially-varying observing conditions in DES Science Verification data

B. Leistedt, H. V. Peiris, F. Elsner +92

Spatially-varying depth and characteristics of observing conditions, such as seeing, airmass, or sky background, are major sources of systematic uncertainties in modern galaxy surv…

astro-ph.CO2015★ 178 cited

Cosmology from Cosmic Shear with DES Science Verification Data

The Dark Energy Survey Collaboration, T. Abbott, F. B. Abdalla +126

We present the first constraints on cosmology from the Dark Energy Survey (DES), using weak lensing measurements from the preliminary Science Verification (SV) data. We use 139 squ…

astro-ph.CO2015★ 119 cited

CMB lensing tomography with the DES Science Verification galaxies

T. Giannantonio, P. Fosalba, R. Cawthon +101

We measure the cross-correlation between the galaxy density in the Dark Energy Survey (DES) Science Verification data and the lensing of the cosmic microwave background (CMB) as re…

astro-ph.CO2015★ 3 cited

Weak lensing by galaxy troughs in DES Science Verification data

D. Gruen, O. Friedrich, A. Amara +89

We measure the weak lensing shear around galaxy troughs, i.e. the radial alignment of background galaxies relative to underdensities in projections of the foreground galaxy field o…