activity
20172021
most citedPredicted Stellar Kinematics of a Kiloparsec-Scale Nuclear Disc (or Ring) in the Milky Way

14 citations · 35 across the 4 of their papers we have counts for

collaborators

6 papers

cs.CV20212 cited

Sub-pixel face landmarks using heatmaps and a bag of tricks

Samuel W. F. Earp, Aubin Samacoits, Sanjana Jain +2

Accurate face landmark localization is an essential part of face recognition, reconstruction and morphing. To accurately localize face landmarks, we present our heatmap regression…

cs.CV20199 cited

Face Detection with Feature Pyramids and Landmarks

Samuel W. F. Earp, Pavit Noinongyao, Justin A. Cairns +1

Accurate face detection and facial landmark localization are crucial to any face recognition system. We present a series of three single-stage RCNNs with different sized backbones…

astro-ph.GA2019

Drivers of disc tilting I: Correlations and possible drivers for Milky Way analogues

Samuel W. F. Earp, Victor P. Debattista, Andrea V. Macciò +3

The direction of the spin vectors of disk galaxies change over time. We present the tilting rate of a sample of galaxies in the NIHAO suite of cosmological hydrodynamical simulatio…

astro-ph.GA2018

The Formation of Compact Elliptical Galaxies in The Vicinity of A Massive Galaxy: The Role of Ram-pressure Confinement

Min Du, Victor P. Debattista, Luis C. Ho +9

Compact ellipticals (cEs) are outliers from the scaling relations of early-type galaxies, particularly the mass-metallicity relation which is an important outcome of feedback. The…

astro-ph.GA201714 cited

Predicted Stellar Kinematics of a Kiloparsec-Scale Nuclear Disc (or Ring) in the Milky Way

Victor P. Debattista, Samuel W. F. Earp, Melissa Ness +1

In Debattista et al. (2015), we proposed that a kiloparsec-scale nuclear disc is responsible for the high-velocity secondary peak in the stellar line-of-sight velocity distribution…

astro-ph.GA201710 cited

The tilting rate of the Milky Way's disc

Samuel W. F. Earp, Victor P. Debattista, Andrea V. Macciò +1

We present tilting rates for galaxies comparable to the Milky Way (MW) in a cold dark matter cosmological hydrodynamical simulation, and compare these with the predicted tiltin…