681 citations · 3.4k across the 38 of their papers we have counts for
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Galaxy and Mass Assembly (GAMA): Fine filaments of galaxies detected within voids
Mehmet Alpaslan, Aaron S. G. Robotham, Danail Obreschkow +15
Based on data from the Galaxy and Mass Assembly (GAMA) survey, we report on the discovery of structures that we refer to as `tendrils' of galaxies: coherent, thin chains of galaxie…
Galaxy And Mass Assembly (GAMA): Spectroscopic analysis
A. M. Hopkins, S. P. Driver, S. Brough +79
The Galaxy And Mass Assembly (GAMA) survey is a multiwavelength photometric and spectroscopic survey, using the AAOmega spectrograph on the Anglo-Australian Telescope to obtain spe…
Hubble Space Telescope survey of the Perseus Cluster -IV: Compact stellar systems in the Perseus Cluster core and Ultra Compact Dwarf formation in star forming filaments
Samantha J. Penny, Duncan A. Forbes, Christopher J. Conselice
We present the results of the first search for Ultra Compact Dwarfs (UCDs) in the Perseus Cluster core, including the region of the cluster around the unusual Brightest Cluster Gal…
Dwarf Galaxies in Clusters as Probes of Galaxy Formation and Dark Matter
Samantha J. Penny, Christopher J. Conselice
We present the results of a Hubble Space Telescope (HST) ACS and WFPC2 study of dwarf galaxies in the nearby Perseus Cluster, down to M_V = -12, spanning the core and outer regions…
Hubble Space Telescope survey of the Perseus Cluster -III: The effect of local environment on dwarf galaxies
Samantha J. Penny, Christopher J. Conselice, Sven De Rijcke +3
We present the results of a Hubble Space Telescope (HST) study of dwarf galaxies in the outer regions of the nearby rich Perseus Cluster, down to M_V = -12, and compare these with…
Smooth, undisturbed dwarf spheroidal galaxies in the Perseus Cluster core: Implications for dark matter content
Samantha J. Penny, Christopher J. Conselice, Sven De Rijcke +1
Using deep HST/ACS observations of the core of the Perseus Cluster, we identify a large population of dwarf elliptical galaxies down to M_V = -12. All these dwarfs are remarkably s…