activity
20162024
most citedHow do central and satellite galaxies quench? -- Insights from spatially resolved spectroscopy in the MaNGA survey

144 citations · 976 across the 23 of their papers we have counts for

collaborators
Showing 2019Show all

7 papers · 1 filter

astro-ph.GA2019★ 79 cited

The ALMaQUEST Survey: III. Scatter in the resolved star forming main sequence is primarily due to variations in star formation efficiency

Sara L. Ellison, Mallory D. Thorp, Lihwai Lin +6

Using a sample of 11,478 spaxels in 34 galaxies with molecular gas, star formation and stellar maps taken from the ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we in…

astro-ph.GA2019★ 138 cited

Are galactic star formation and quenching governed by local, global or environmental phenomena?

Asa F. L. Bluck, Roberto Maiolino, Sebastian Sanchez +5

We present an analysis of star formation and quenching in the SDSS-IV MaNGA-DR15, utilising over 5 million spaxels from 3500 local galaxies. We estimate star formation rate s…

astro-ph.GA2019★ 117 cited

Deep learning predictions of galaxy merger stage and the importance of observational realism

Connor Bottrell, Maan H. Hani, Hossen Teimoorinia +7

Machine learning is becoming a popular tool to quantify galaxy morphologies and identify mergers. However, this technique relies on using an appropriate set of training data to be…

astro-ph.IM2019★ 2 cited

LRP2020: Machine Learning Advantages in Canadian Astrophysics

K. A. Venn, S. Fabbro, A Liu +12

The application of machine learning (ML) methods to the analysis of astrophysical datasets is on the rise, particularly as the computing power and complex algorithms become more po…

astro-ph.GA2019

Dwarfs or giants? Stellar metallicities and distances in the Canada-France-Imaging-Survey from multi-band photometry

Guillaume F. Thomas, Nicholaas Annau, Alan McConnachie +19

We present a new fully data-driven algorithm that uses photometric data from the Canada-France-Imaging-Survey (CFIS; ), Pan-STARRS 1 (PS1; ), and Gaia () to discriminat…

astro-ph.SR2019★ 4 cited

CLOVER: Convnet Line-fitting Of Velocities in Emission-line Regions

Jared Keown, James Di Francesco, Hossen Teimoorinia +2

When multiple star-forming gas structures overlap along the line-of-sight and emit optically thin emission at significantly different radial velocities, the emission can become non…

astro-ph.GA2019★ 70 cited

What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure

Asa F. L. Bluck, Connor Bottrell, Hossen Teimoorinia +9

We investigate the dependence of galaxy structure on a variety of galactic and environmental parameters for ~500,000 galaxies at z<0.2, taken from the Sloan Digital Sky Survey data…