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20092026
most citedGalaxy and Mass Assembly (GAMA): survey diagnostics and core data release

1.1k citations · 11.2k across the 112 of their papers we have counts for

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Showing 2014Show all

11 papers · 1 filter

astro-ph.GA2014★ 297 cited

Galaxy And Mass Assembly (GAMA): mass-size relations of z0.1 galaxies subdivided by Sérsic index, colour and morphology

Rebecca Lange, Simon P. Driver, Aaron S. G. Robotham +20

We use data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01z0.1 (8399 galaxies in to bands) to derive the stellar mass half-light rad…

astro-ph.GA2014★ 24 cited

Galaxy And Mass Assembly (GAMA): Bivariate functions of H star forming galaxies

M. L. P. Gunawardhana, A. M. Hopkins, E. N. Taylor +18

We present bivariate luminosity and stellar mass functions of H star forming galaxies drawn from the Galaxy And Mass Assembly (GAMA) survey. While optically deep spectroscopic o…

astro-ph.GA2014★ 18 cited

Galaxy And Mass Assembly (GAMA): The unimodal nature of the dwarf galaxy population

Smriti Mahajan, Michael J. Drinkwater, S. Driver +9

In this paper we aim to (i) test the number of statistically distinct classes required to classify the local galaxy population, and, (ii) identify the differences in the physical a…

astro-ph.GA2014★ 105 cited

Galaxy And Mass Assembly (GAMA): Refining the Local Galaxy Merger Rate using Morphological Information

Kevin R. V. Casteels, Christopher J. Conselice, Steven P. Bamford +16

We use the Galaxy And Mass Assembly (GAMA) survey to measure the local Universe mass dependent merger fraction and merger rate using galaxy pairs and the CAS structural method, whi…

astro-ph.GA2014★ 140 cited

Galaxy And Mass Assembly: Deconstructing Bimodality - I. Red ones and blue ones

Edward N. Taylor, Andrew M. Hopkins, Ivan K. Baldry +18

We measure the mass functions for generically red and blue galaxies, using a z < 0.12 sample of log M* > 8.7 field galaxies from the Galaxy And Mass Assembly (GAMA) survey. Our mot…

astro-ph.GA2014★ 165 cited

Galaxy And Mass Assembly (GAMA): Galaxy close-pairs, mergers, and the future fate of stellar mass

A. S. G. Robotham, S. P. Driver, L. J. M. Davies +28

We use a highly complete subset of the GAMA-II redshift sample to fully describe the stellar mass dependence of close-pairs and mergers between 10^8 Msun and 10^12 Msun. Using the…

astro-ph.GA2014★ 135 cited

Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type

Lee S. Kelvin, Simon P. Driver, Aaron S. G. Robotham +22

We present an estimate of the galaxy stellar mass function and its division by morphological type in the local (0.025 < z < 0.06) Universe. Adopting robust morphological classifica…

astro-ph.GA2014★ 22 cited

Galaxy and Mass Assembly (GAMA): merging galaxies and their properties

Roberto De Propris, Ivan K. Baldry, Joss Bland-Hawthorn +7

We derive the close pair fractions and volume merger rates as a function of luminosity and morphology for galaxies in the GAMA survey with -23 < M(r) < -17 at 0.01 < z < 0.22. The…

astro-ph.IM2014★ 142 cited

Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors

I. K. Baldry, M. Alpaslan, A. E. Bauer +17

The Galaxy And Mass Assembly (GAMA) survey has obtained spectra of over 230000 targets using the Anglo-Australian Telescope. To homogenise the redshift measurements and improve the…

astro-ph.CO2014★ 91 cited

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…

astro-ph.CO2014★ 93 cited

Galaxy And Mass Assembly (GAMA): ugrizYJHK Sérsic luminosity functions and the cosmic spectral energy distribution by Hubble type

Lee S. Kelvin, Simon P. Driver, Aaron S. G. Robotham +20

We report the morphological classification of 3727 galaxies from the Galaxy and Mass Assembly survey with M_r < -17.4 mag and in the redshift range 0.025 < z < 0.06 (2.1 x 10^5 Mpc…