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20172025
most citedThe SAMI Galaxy Survey: A Range in S0 Properties Indicating Multiple Formation Pathways

42 citations · 118 across the 5 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2025

The coherent satellite velocity field around the interacting spiral galaxy pair NGC5713/19: signature of two galaxy groups merging

Helmut Jerjen, Simon Deeley, Holger Baumgardt +1

The luminous spirals NGC5713 and NGC5719 form an interacting galaxy pair 94 kpc apart and are connected by a straight, elongated neutral hydrogen structure extending over 200 kpc.…

astro-ph.GA202142 cited

The two formation pathways of S0 galaxies

Simon Deeley, Michael J. Drinkwater, Sarah M. Sweet +4

Despite their ubiquity throughout the Universe, the formation of S0 galaxies remains uncertain. Recent observations have revealed that S0 galaxies make up a diverse population whic…

astro-ph.GA202042 cited

The SAMI Galaxy Survey: A Range in S0 Properties Indicating Multiple Formation Pathways

Simon Deeley, Michael J. Drinkwater, Sarah M. Sweet +14

It has been proposed that S0 galaxies are either fading spirals or the result of galaxy mergers. The relative contribution of each pathway, and the environments in which they occur…

astro-ph.GA201912 cited

Classifying the formation processes of S0 galaxies using Convolutional Neural Networks

J. D. Diaz, Kenji Bekki, Duncan A. Forbes +3

Numerous studies have demonstrated the ability of Convolutional Neural Networks (CNNs) to classify large numbers of galaxies in a manner which mimics the expertise of astronomers.…

astro-ph.GA2018

Formation of S0s via disc accretion around high-redshift compact ellipticals

J. D. Diaz, Kenji Bekki, Duncan A. Forbes +3

We present hydrodynamical N-body models which demonstrate that elliptical galaxies can transform into S0s by acquiring a disc. In particular, we show that the merger with a massive…

astro-ph.GA2018

Galaxy Tagging: photometric redshift refinement and group richness enhancement

P. R. Kafle, A. S. G. Robotham, S. P. Driver +4

We present a new scheme, , for refining the photometric redshift measurements of faint galaxies by probabilistically tagging them to observed galaxy groups constructed…