activity
20132016
most citedAngular Momenta, Dynamical Masses, and Mergers of Brightest Cluster Galaxies

46 citations · 171 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2016★ 16 cited

A Study of Central Galaxy Rotation with Stellar Mass and Environment

Paola Oliva-Altamirano, Sarah Brough, Kim-Vy Tran +11

We present a pilot analysis of the influence of galaxy stellar mass and cluster environment on the probability of slow rotation in 22 central galaxies at mean redshift . Th…

astro-ph.GA2016★ 7 cited

Spatial Correlation Between Dust and H Emission in Dwarf Irregular Galaxies

Jimmy, Kim-Vy Tran, Amélie Saintonge +5

Using a sample of dwarf irregular galaxies selected from the ALFALFA blind HI-survey and observed using the VIMOS IFU, we investigate the relationship between H emission and Bal…

astro-ph.GA2015★ 33 cited

The Gas Phase Mass Metallicity Relation for Dwarf Galaxies: Dependence on Star Formation Rate and HI Gas Mass

Jimmy, Kim-Vy Tran, Amélie Saintonge +3

Using a sample of dwarf galaxies observed using the VIMOS IFU on the VLT, we investigate the mass-metallicity relation (MZR) as a function of star formation rate (FMR$_{\text{SFR}}…

astro-ph.GA2015★ 33 cited

The accretion histories of brightest cluster galaxies from their stellar population gradients

Paola Oliva-Altamirano, Sarah Brough, Jimmy +6

We analyse the spatially-resolved stellar populations of 9 local () Brightest Cluster Galaxies (BCGs) observed with VIMOS in IFU mode. Our sample is composed of 7 slow-rotat…

hep-ph2015★ 1 cited

Decoupled Sectors and Wolf-Rayet Galaxies

Willy Fischler, Jimmy, Dustin Lorshbough

It has recently been proposed that gamma-ray burst (GRB) events may be modified by the presence of a dark matter sector subcomponent that is charged under an unbroken U(1). This pr…

astro-ph.GA2014★ 35 cited

Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures

Davide Martizzi, Jimmy, Romain Teyssier +1

A large sample of cosmological hydrodynamical zoom-in simulations with Adaptive Mesh Refinement (AMR) is analysed to study the properties of simulated Brightest Cluster Galaxies (B…

astro-ph.GA2013★ 46 cited

Angular Momenta, Dynamical Masses, and Mergers of Brightest Cluster Galaxies

Jimmy, Kim-Vy Tran, Sarah Brough +4

Using the VIMOS Integral Field Unit (IFU) spectrograph on the Very Large Telescope (VLT), we have spatially mapped the kinematic properties of 10 nearby Brightest Cluster Galaxies…