output
20042026
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations

Showing 2017Show all

20 papers · 1 filter

astro-ph.GA2017246 cited

Galaxy growth in a massive halo in the first billion years of cosmic history

D. P. Marrone, J. S. Spilker, C. C. Hayward +34

According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in reg…

astro-ph.HE2017116 cited

Solar abundance ratios of the iron-peak elements in the Perseus Cluster

Hitomi Collaboration

The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray spectroscopy…

astro-ph.GA201711 cited

The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way

B. B. Thompson, C. G. Few, M. Bergemann +39

The typical methodology for comparing simulated galaxies with observational surveys is usually to apply a spatial selection to the simulation to mimic the region of interest covere…

nucl-ex201743 cited

Halo-induced large enhancement of soft dipole excitation of 11Li observed via proton inelastic scattering

Junki Tanaka

Proton inelastic scattering off a neutron halo nucleus, 11Li, has been studied in inverse kinematics at the IRIS facility at TRIUMF. The aim was to establish a soft dipole resonanc…

astro-ph.GA201723 cited

Chemical Mapping of the Milky Way With The Canada-France Imaging Survey: A Non-parametric Metallicity-Distance Decomposition of the Galaxy

Rodrigo Ibata, Alan McConnachie, Jean-Charles Cuillandre +41

We present the chemical distribution of the Milky Way, based on 2,900 of -band photometry taken as part of the Canada-France Imaging Survey. When complete, this…

astro-ph.GA2017103 cited

The Canada-France Imaging Survey: First results from the u-band component

Rodrigo Ibata, Alan McConnachie, Jean-Charles Cuillandre +41

The Canada-France Imaging Survey (CFIS) will map the northern high Galactic latitude sky in the -band ("CFIS-u", 10,000) and in the -band ("CFIS-r", 5,000$\,…