output
20022026
most citedThe electronic properties of graphene

24.8k citations

Showing 2022 · astro-ph.GAShow all

12 papers · 2 filters

astro-ph.GA2022★ 18 cited

Multiple shock fronts in RBS 797: the Chandra window on shock heating in galaxy clusters

F. Ubertosi, M. Gitti, F. Brighenti +11

Using 427 ks of Chandra observations, we present a study of shock heating and ICM cooling in the galaxy cluster RBS 797. We discover three nested pairs of weak shocks at roug…

astro-ph.GA2022★ 10 cited

DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at

David J. Setton, Biprateep Dey, Gourav Khullar +24

We utilize bright Luminous Red Galaxies (LRGs) from the novel Dark Energy Spectroscopic Instrument Survey Validation spectroscopic sample, leveraging its deep ($\sim2.5…

astro-ph.GA2022★ 4 cited

The VST ATLAS Quasar Survey I: Catalogue

Alice Eltvedt, T. Shanks, N. Metcalfe +22

We present the VST ATLAS Quasar Survey, consisting of quasar (QSO) candidates with over deg. The catalogue is based on VST ATLASNEOWIS…

astro-ph.GA2022★ 12 cited

HST and HSC Weak-lensing Study of the Equal-mass Dissociative Merger CIZA J0107.7+5408

Kyle Finner, Scott W. Randall, M. James Jee +6

A dissociative merger is formed by the interplay of ram pressure and gravitational forces, which can lead to a spatial displacement of the dark matter and baryonic components of th…

astro-ph.GA2022★ 14 cited

Gas sloshing and cold fronts in pre-merging galaxy cluster Abell 98

Arnab Sarkar, Scott Randall, Yuanyuan Su +10

We present deep Chandra observations of the pre-merger galaxy cluster Abell 98. Abell 98 is a complex merging system. While the northern (A98N) and central subclusters (A98S) are m…

astro-ph.GA2022★ 10 cited

Living on the edge of the Central Molecular Zone: G1.3 is the more likely candidate for gas accretion into the CMZ

Laura A. Busch, Denise Riquelme, Rolf Güsten +3

The 1.3deg (G1.3) and 1.6deg (G1.6) cloud complexes in the Central Molecular Zone (CMZ) of our Galaxy have been proposed to possibly reside at the intersection region of the X1 and…