activity
20072019
most citedThe Gaia-ESO Survey: Kinematic structure in the Gamma Velorum Cluster

133 citations · 745 across the 15 of their papers we have counts for

collaborators

15 papers

physics.med-ph2019★ 1 cited

Modelling an equivalent b-value in diffusion-weighted steady-state free precession

Benjamin C. Tendler, Sean Foxley, Michiel Cottaar +2

Purpose: Diffusion-weighted steady-state free precession (DW-SSFP) is shown to provide a means to probe non-Gaussian diffusion through manipulation of the flip angle. A framework i…

physics.med-ph2019★ 20 cited

Improved fibre dispersion estimation using b-tensor encoding

Michiel Cottaar, Filip Szczepankiewicz, Matteo Bastiani +4

Measuring fibre dispersion in white matter with diffusion magnetic resonance imaging (MRI) is limited by an inherent degeneracy between fibre dispersion and microscopic diffusion a…

astro-ph.SR2017★ 35 cited

IN-SYNC VI. Identification and Radial Velocity Extraction for 100+ Double-Lined Spectroscopic Binaries in the APOGEE/IN-SYNC Fields

M. A. Fernandez, Kevin R. Covey, Nathan De Lee +15

We present radial velocity measurements for 70 high confidence, and 34 potential binary systems in fields containing the Perseus Molecular Cloud, Pleiades, NGC 2264, and the Orion…

astro-ph.GA2017★ 59 cited

IN-SYNC. V. Stellar kinematics and dynamics in the Orion A Molecular Cloud

Nicola Da Rio, Jonathan C. Tan, Kevin R. Covey +14

The kinematics and dynamics of young stellar populations enable us to test theories of star formation. With this aim, we continue our analysis of the SDSS-III/APOGEE IN-SYNC survey…

astro-ph.GA2015★ 110 cited

IN-SYNC IV - The Young Stellar Population in the Orion A Molecular Cloud

Nicola Da Rio, Jonathan C. Tan, Kevin R. Covey +14

We present the results of the SDSS APOGEE INfrared Spectroscopy of Young Nebulous Clusters program (IN-SYNC) survey of the Orion A molecular cloud. This survey obtained high resolu…

astro-ph.SR2015

IN-SYNC III: The dynamical state of IC 348 - A super-virial velocity dispersion and a puzzling sign of convergence

Michiel Cottaar, Kevin R. Covey, Jonathan B. Foster +11

Most field stars will have encountered the highest stellar density and hence the largest number of interactions in their birth environment. Yet the stellar dynamics during this cru…