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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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60 papers · 1 filter

astro-ph.GA2024

The Galaxy Zoo Catalogs for the Galaxy And Mass Assembly (GAMA) Survey

Benne W. Holwerda, Clayton Robertson, Kyle Cook +16

Galaxy Zoo is an online project to classify morphological features in extra-galactic imaging surveys with public voting. In this paper, we compare the classifications made for two…

astro-ph.GA2024

Merian: A Wide-Field Imaging Survey of Dwarf Galaxies at z~0.06-0.10

Shany Danieli, Erin Kado-Fong, Song Huang +32

We present the Merian Survey, an optical imaging survey optimized for studying the physical properties of bright star-forming dwarf galaxies. Merian is carried out with two medium-…

astro-ph.GA2024★ 19 cited

Strategies for optimal sky subtraction in the low surface brightness regime

A. E. Watkins, S. Kaviraj, C. C. Collins +5

The low surface brightness (LSB) regime ( mag arcsec) comprises a vast, mostly unexplored discovery space, from dwarf galaxies to the diffuse interstellar…

astro-ph.GA2023★ 32 cited

An almost dark galaxy with the mass of the Small Magellanic Cloud

Mireia Montes, Ignacio Trujillo, Ananthan Karunakaran +9

Almost Dark Galaxies are objects that have eluded detection by traditional surveys such as the Sloan Digital Sky Survey (SDSS). The low surface brightness of these galaxies ((…

astro-ph.GA2023★ 15 cited

The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing

Yifei Luo, Alexie Leauthaud, Jenny Greene +28

The Merian survey is mapping 850 degrees of the Hyper Suprime-Cam Strategic Survey Program (HSC-SSP) wide layer with two medium-band filters on the 4-meter Victor M. Bla…

astro-ph.GA2023★ 9 cited

The Loneliest Galaxies in the Universe: A GAMA and GalaxyZoo Study on Void Galaxy Morphology

Lori E. Porter, Benne W. Holwerda, Sandor Kruk +5

The large-scale structure (LSS) of the Universe is comprised of galaxy filaments, tendrils, and voids. The majority of the Universe's volume is taken up by these voids, which exist…

astro-ph.GA2022

Galaxy And Mass Assembly: Galaxy Morphology in the Green Valley, Prominent rings and looser Spiral Arms

Dominic Smith, Lutz Haberzettl, L. E. Porter +15

Galaxies broadly fall into two categories: star-forming (blue) galaxies and quiescent (red) galaxies. In between, one finds the less populated ``green valley". Some of these galaxi…

astro-ph.GA2022★ 28 cited

Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe

Sarah Casura, Jochen Liske, Aaron S. G. Robotham +10

We derive single Sérsic fits and bulge-disk decompositions for 13096 galaxies at redshifts z < 0.08 in the GAMA II equatorial survey regions in the Kilo-Degree Survey (KiDS) g, r a…

astro-ph.GA2022★ 48 cited

Galapagos-2/Galfitm/GAMA -- multi-wavelength measurement of galaxy structure: separating the properties of spheroid and disk components in modern surveys

Boris Häußler, Marina Vika, Steven P. Bamford +6

We present the capabilities of Galapagos--2 and Galfitm in the context of fitting 2-component profiles to galaxies, on the way to providing complete multi-band, multi-component fit…

astro-ph.GA2022★ 11 cited

Galaxy And Mass Assembly (GAMA): Self-Organizing Map Application on Nearby Galaxies

B. W. Holwerda, Dominic Smith, Lori Porter +12

Galaxy populations show bimodality in a variety of properties: stellar mass, colour, specific star-formation rate, size, and Sérsic index. These parameters are our feature space. W…

astro-ph.GA2022★ 249 cited

Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

Simon P. Driver, Sabine Bellstedt, Aaron S. G. Robotham +67

In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earli…

astro-ph.GA2022★ 33 cited

North Ecliptic Pole merging galaxy catalogue

W. J. Pearson, L. E. Suelves, S. C. -C. Ho +17

We aim to generate a catalogue of merging galaxies within the 5.4 sq. deg. North Ecliptic Pole over the redshift range . To do this, imaging data from the Hyper Supr…

astro-ph.GA2021★ 201 cited

Galaxy Zoo DECaLS: Detailed Visual Morphology Measurements from Volunteers and Deep Learning for 314,000 Galaxies

Mike Walmsley, Chris Lintott, Tobias Geron +15

We present Galaxy Zoo DECaLS: detailed visual morphological classifications for Dark Energy Camera Legacy Survey images of galaxies within the SDSS DR8 footprint. Deeper DECaLS ima…

astro-ph.GA2021★ 56 cited

The Growth of Intracluster Light in XCS-HSC Galaxy Clusters from

Kate E. Furnell, Chris A. Collins, Lee S. Kelvin +14

We estimate the Intracluster Light (ICL) component within a sample of 18 clusters detected in XMM Cluster Survey (XCS) data using deep ( 26.8 mag) Hyper Suprime Cam Subaru St…

astro-ph.GA2020

Galaxy And Mass Assembly: A Comparison between Galaxy-Galaxy Lens Searches in KiDS/GAMA

Shawn Knabel, Rebecca L. Steele, Benne W. Holwerda +9

Strong gravitational lenses are a rare and instructive type of astronomical object. Identification has long relied on serendipity, but different strategies -- such as mixed spectro…

astro-ph.GA2020★ 29 cited

GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation

Edward N. Taylor, Michelle E. Cluver, Alan Duffy +16

We use KiDS weak lensing data to measure variations in mean halo mass as a function of several key galaxy properties (namely: stellar colour, specific star formation rate, Sersic i…

astro-ph.GA2019★ 22 cited

The frequency of dust lanes in edge-on spiral galaxies identified by Galaxy Zoo in KiDS imaging of GAMA targets

B. W. Holwerda, L. Kelvin, I. Baldry +20

Dust lanes bisect the plane of a typical edge-on spiral galaxy as a dark optical absorption feature. Their appearance is linked to the gravitational stability of spiral disks; the…

astro-ph.GA2019★ 4 cited

The galaxy stellar mass function from CCSNe with improved photo-z techniques

Thomas M. Sedgwick, Ivan K. Baldry, Philip A. James +1

In Sedgwick et al. (2019) we introduced and utilised a method to combat surface brightness and mass biases in galaxy sample selection, using core-collapse supernovae (CCSNe) as poi…

astro-ph.GA2019★ 36 cited

Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65

G. Erfanianfar, A. Finoguenov, K. Furnell +25

We present the brightest cluster galaxies (BCGs) catalog for SPectroscoic IDentification of eROSITA Sources (SPIDERS) DR14 cluster program value-added catalog. We list the 416 BCGs…

astro-ph.GA2019★ 14 cited

The Galaxy Stellar Mass Function and Low Surface Brightness Galaxies from Core-Collapse Supernovae

Thomas M. Sedgwick, Ivan K. Baldry, Philip A. James +1

We introduce a method for producing a galaxy sample unbiased by surface brightness and stellar mass, by selecting star-forming galaxies via the positions of core-collapse supernova…

astro-ph.GA2018★ 47 cited

Testing Convolutional Neural Networks for finding strong gravitational lenses in KiDS

C. E. Petrillo, C. Tortora, S. Chatterjee +7

Convolutional Neural Networks (ConvNets) are one of the most promising methods for identifying strong gravitational lens candidates in survey data. We present two ConvNet lens-find…

astro-ph.GA2018★ 38 cited

Galaxy and Mass Assembly (GAMA): Variation in Galaxy Structure Across the Green Valley

Lee S. Kelvin, Malcolm N. Bremer, Steven Phillipps +26

Using a sample of 472 local Universe (z<0.06) galaxies in the stellar mass range 10.25 < log M*/M_sun < 10.75, we explore the variation in galaxy structure as a function of morphol…

astro-ph.GA2018★ 19 cited

Exploring Relations Between BCG \& Cluster Properties in the SPectroscopic IDentification of eROSITA Sources Survey from

Kate E. Furnell, Chris A. Collins, Lee S. Kelvin +6

We present a sample of 329 low to intermediate redshift () brightest cluster galaxies (BCGs) in X-ray selected clusters from the SPectroscopic IDentification of eRo…

astro-ph.GA2018★ 88 cited

Galaxy and Mass Assembly (GAMA): Morphological transformation of galaxies across the green valley

M. N. Bremer, S. Phillipps, L. S. Kelvin +13

We explore constraints on the joint photometric and morphological evolution of typical low redshift galaxies as they move from the blue cloud through the green valley and onto the…