activity
19992022
most citedBilby: A user-friendly Bayesian inference library for gravitational-wave astronomy

1.1k citations · 6.5k across the 86 of their papers we have counts for

collaborators
Showing 2020Show all

15 papers · 1 filter

astro-ph.GA2020★ 12 cited

The SAMI Galaxy Survey: Kinematics of stars and gas in brightest group galaxies; the role of group dynamics

Mojtaba Raouf, Rory Smith, Habib G. Khosroshahi +17

We study the stellar and gas kinematics of the brightest group galaxies (BGGs) in dynamically relaxed and unrelaxed galaxy groups for a sample of 154 galaxies in the SAMI galaxy su…

astro-ph.GA2020★ 5 cited

The Sami Galaxy Survey: stellar populations of passive spiral galaxies in different environment

Mina Pak, Sree Oh, Joon Hyeop Lee +17

We investigate the stellar populations of passive spiral galaxies as a function of mass and environment, using integral field spectroscopy data from the Sydney-AAO Multi-object Int…

astro-ph.GA2020★ 60 cited

GASP XXIX -- Unwinding the arms of spiral galaxies via ram-pressure stripping

Callum Bellhouse, Sean L. McGee, Rory Smith +11

We present the first study of the effect of ram-pressure "unwinding" the spiral arms of cluster galaxies. We study 11 ram-pressure stripped galaxies from GASP (GAs Stripping Phenom…

gr-qc2020★ 24 cited

Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model

Tousif Islam, Scott E. Field, Carl-Johan Haster +1

The recent observation of GW190412, the first high-mass ratio binary black-hole (BBH) merger, by the LIGO-Virgo Collaboration (LVC) provides a unique opportunity to probe the impac…

gr-qc2020★ 230 cited

GW190521 as a merger of Proca stars: a potential new vector boson of eV

Juan Calderón Bustillo, Nicolas Sanchis-Gual, Alejandro Torres-Forné +6

Advanced LIGO-Virgo reported a short gravitational-wave signal (GW190521) interpreted as a quasi-circular merger of black holes, one populating the pair-instability supernova gap,…

astro-ph.HE2020★ 65 cited

Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds

Sylvia Biscoveanu, Colm Talbot, Eric Thrane +1

Primordial gravitational waves are expected to create a stochastic background encoding information about the early Universe that may not be accessible by other means. However, the…

astro-ph.GA2020★ 45 cited

Beyond halo mass: quenching galaxy mass assembly at the edge of filaments

Hyunmi Song, Clotilde Laigle, Ho Seong Hwang +6

We examine how the mass assembly of central galaxies depends on their location in the cosmic web. The HORIZON-AGN simulation is analysed at z~2 using the DISPERSE code to extract m…

astro-ph.HE2020★ 49 cited

A scalable random forest regressor for combining neutron-star equation of state measurements: A case study with GW170817 and GW190425

Francisco Hernandez Vivanco, Rory Smith, Eric Thrane +1

Gravitational-wave observations of binary neutron star coalescences constrain the neutron-star equation of state by enabling measurement of the tidal deformation of each neutron st…

astro-ph.GA2020

The Blue Compact Dwarf Galaxy VCC 848 Formed by Dwarf-Dwarf Merging: HI Gas, Star Formation and Numerical Simulations

Hong-Xin Zhang, Rory Smith, Se-Heon Oh +12

A clear link between a dwarf-dwarf merger event and enhanced star formation (SF) in the recent past was recently identified in the gas-dominated merger remnant VCC 848, offering by…

astro-ph.GA2020★ 12 cited

Revealing the formation mechanism of the shell galaxy NGC474 with MUSE

Jeremy Fensch, Pierre-Alain Duc, Sungsoon Lim +6

Stellar shells around galaxies could provide precious insights into their assembly history. However, their formation mechanism remains poorly empirically constrained, in particular…

astro-ph.GA2020★ 13 cited

Toward Solving the Puzzle: Dissecting the Complex Merger A521 with Multi-wavelength Data

Mijin Yoon, Wonki Lee, M. James Jee +3

A521 has been a subject of extensive panchromatic studies from X-ray to radio. The cluster possesses a number of remarkable features including a bright radio relic with a steep spe…

astro-ph.HE2020★ 28 cited

Inferring the population properties of binary black holes from unresolved gravitational waves

Rory Smith, Colm Talbot, Francisco Hernandez Vivanco +1

The vast majority of compact binary mergers in the Universe produce gravitational waves that are too weak to yield unambiguous detections; they are unresolved. We present a method…

astro-ph.GA2020★ 33 cited

The Blue Compact Dwarf Galaxy VCC848 Formed by Dwarf-Dwarf Merging

Hong-Xin Zhang, Sanjaya Paudel, Rory Smith +8

It has long been speculated that many starburst or compact dwarf galaxies are resulted from dwarf-dwarf galaxy merging, but unequivocal evidence for this possibility has rarely bee…

astro-ph.GA2020★ 52 cited

YZiCS: Unveiling Quenching History of Cluster Galaxies Using Phase-space Analysis

Jinsu Rhee, Rory Smith, Hoseung Choi +4

We used the time since infall (TSI) of galaxies, obtained from the Yonsei Zoom-in Cluster Simulation, and the star formation rate (SFR) from the Sloan Digital Sky Survey (SDSS) Dat…

physics.ins-det2020★ 11 cited

An analysis and visualization of the output mode-matching requirements for squeezing in Advanced LIGO and future gravitational wave detectors

Antonio Perreca, Aidan Brooks, Jonathan Richardson +2

The sensitivity of ground-based gravitational wave (GW) detectors will be improved in the future via the injection of frequency-dependent squeezed vacuum. The achievable improvemen…