activity
20062022
most citedVERTICO: The Virgo Environment Traced In CO Survey

68 citations · 286 across the 17 of their papers we have counts for

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Showing 2019Show all

11 papers · 1 filter

astro-ph.GA20197 cited

The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological Simulations

Kyungwon Chun, Rory Smith, Jihye Shin +2

Using high resolution hydrodynamical cosmological simulations, we study the gas accretion history of low mass halos located in a field-like, low density environment. We track their…

astro-ph.GA201917 cited

The impact of the dynamical state of galaxy groups on the stellar populations of central galaxies

Mojtaba Raouf, Rory Smith, Habib G. Khosroshahi +4

We study the stellar populations of the brightest group galaxies (BGGs) in groups with different dynamical states, using GAMA survey data. We use two independent, luminosity depend…

astro-ph.GA201919 cited

Leavers and remainers: Galaxies split by group-exit

Nelvy Choque-Challapa, Rory Smith, Graeme Candlish +2

The disruption of substructure in galaxy clusters likely plays an important role in shaping the cluster population as a significant fraction of cluster galaxies today have spent ti…

gr-qc201923 cited

Gravitational wave detection without boot straps: a Bayesian approach

Gregory Ashton, Eric Thrane, Rory J. E. Smith

In order to separate astrophysical gravitational-wave signals from instrumental noise, which often contains transient non-Gaussian artifacts, astronomers have traditionally relied…

gr-qc2019

Massively parallel Bayesian inference for transient gravitational-wave astronomy

Rory Smith, Gregory Ashton, Avi Vajpeyi +1

Understanding the properties of transient gravitational waves and their sources is of broad interest in physics and astronomy. Bayesian inference is the standard framework for astr…

gr-qc2019

Measuring the neutron star equation of state with gravitational waves: the first forty binary neutron star mergers

Francisco Hernandez Vivanco, Rory Smith, Eric Thrane +3

Gravitational waves from binary neutron star coalescences contain rich information about matter at supranuclear densities encoded by the neutron star equation of state. We can meas…