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20042025
most citedGalaxy and Mass Assembly (GAMA): survey diagnostics and core data release

1.1k citations · 6.7k across the 58 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.GA2016★ 42 cited

Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe I. - The Effect of the Group Environment on Star Formation in Spiral Galaxies

M. W. Grootes, R. J. Tuffs, C. C. Popescu +20

Abridged - We quantify the effect of the galaxy group environment (for 12.5 < log(M_group/Msun) < 14.0) on the star formation rates of the (morphologically-selected) population of…

astro-ph.GA2016★ 50 cited

The Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS): Survey design, data catalogue and GAMA/WiggleZ spectroscopy

John H. Y. Ching, Elaine M. Sadler, Scott M. Croom +6

We present the Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS), a spectroscopic catalogue of radio sources designed to include the full range of radio AGN populati…

astro-ph.GA2016★ 107 cited

The SAMI Galaxy Survey: Spatially resolving the environmental quenching of star formation in GAMA galaxies

A. L. Schaefer, S. M. Croom, J. T. Allen +32

We use data from the Sydney-AAO Multi-Object Integral Field Spectrograph (SAMI) Galaxy Survey and the Galaxy And Mass Assembly (GAMA) survey to investigate the spatially-resolved s…

astro-ph.GA2016★ 14 cited

Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations

P. R. Kafle, A. S. G. Robotham, C. del P. Lagos +12

We investigate the contentious issue of the presence, or lack thereof, of satellites mass segregation in galaxy groups using the Galaxy And Mass Assembly (GAMA) survey, the GALFORM…

astro-ph.CO2016★ 46 cited

Evolution of cosmic filaments and of their galaxy population from MHD cosmological simulations

Claudio Gheller, Franco Vazza, Marcus Brueggen +4

Despite containing about a half of the total matter in the Universe, at most wavelengths the filamentary structure of the cosmic web is difficult to observe. In this work, we use l…