Galaxy And Mass Assembly (GAMA): end of survey report and data release 2

Abstract

The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectroscopic surveys of low-redshift galaxies. Covering an area of ~286 deg^2 (split among five survey regions) down to a limiting magnitude of r < 19.8 mag, we have collected spectra and reliable redshifts for 238,000 objects using the AAOmega spectrograph on the Anglo-Australian Telescope. In addition, we have assembled imaging data from a number of independent surveys in order to generate photometry spanning the wavelength range 1 nm - 1 m. Here we report on the recently completed spectroscopic survey and present a series of diagnostics to assess its final state and the quality of the redshift data. We also describe a number of survey aspects and procedures, or updates thereof, including changes to the input catalogue, redshifting and re-redshifting, and the derivation of ultraviolet, optical and near-infrared photometry. Finally, we present the second public release of GAMA data. In this release we provide input catalogue and targeting information, spectra, redshifts, ultraviolet, optical and near-infrared photometry, single-component Sérsic fits, stellar masses, H$\alpha$-derived star formation rates, environment information, and group properties for all galaxies with r < 19.0 mag in two of our survey regions, and for all galaxies with r < 19.4 mag in a third region (72,225 objects in total). The database serving these data is available at http://www.gama-survey.org/.

Accepted for publication in MMRAS, 40 pages, 33 figures

References in corpus (24)

• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• The Cosmic Evolution Survey (COSMOS) -- Overview
• K-corrections and filter transformations in the ultraviolet, optical, and near infrared
• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• The SAMI Galaxy Survey: instrument specification and target selection
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
• Kinematic Structure of Merger Remnants
• The structure of galactic disks: Studying late-type spiral galaxies using SDSS
• The 2dF-SDSS LRG and QSO (2SLAQ) Luminous Red Galaxy Survey
• Galaxy And Mass Assembly (GAMA): Galaxy close-pairs, mergers, and the future fate of stellar mass
• The SAMI Galaxy Survey: Early Data Release
• Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors
• Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type
• The 2dF-SDSS LRG and QSO Survey: The spectroscopic QSO catalogue
• Galaxy And Mass Assembly (GAMA): The galaxy luminosity function within the cosmic web
• Galaxy And Mass Assembly (GAMA): Curation and reanalysis of 16.6k redshifts in the G10/COSMOS region
• Galaxy And Mass Assembly (GAMA): The dependence of the galaxy luminosity function on environment, redshift and colour
• Precision cosmology with a wide area XMM cluster survey
• Galaxy And Mass Assembly (GAMA): Bivariate functions of H$\alpha$ star forming galaxies
• Galaxy And Mass Assembly: Estimating galaxy group masses via caustic analysis
• Galaxy and Mass Assembly (GAMA): maximum likelihood determination of the luminosity function and its evolution

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• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey
• Star-Forming, Rotating Spheroidal Galaxies in the GAMA and SAMI Surveys
• The distribution and properties of DLAs at z $\le$ 2 in the EAGLE simulations
• The OTELO survey: Nature and mass-metallicity relation for H$\alpha$ emitters at $z\sim 0.4$
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Galaxy and Mass Assembly (GAMA): Probing the merger histories of massive galaxies via stellar populations
• Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg${}^2$ at z=0.3-0.6
• Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies
• Galaxy And Mass Assembly (GAMA): The group HI mass as a function of halo mass
• The size--mass and other structural parameter ($n,{\mu }_z,R_z$) relations for local bulges/spheroids from multicomponent decompositions
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• Searching for Dark Matter Signals from Local Dwarf Spheroidal Galaxies at Low Radio Frequencies in the GLEAM Survey
• UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?
• Galaxy classification: A machine learning analysis of GAMA catalogue data
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• FLASH Pilot Survey: Detections of associated 21 cm HI absorption in GAMA galaxies at 0.42 < z <1.00
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Impact of tidal environment on galaxy clustering in GAMA
• Discovery of a Bimodal Environmental Distribution of Compact Ellipticals in the Local Universe
• Galaxy And Mass Assembly: Galaxy Zoo spiral arms and star formation rates
• Relativistic Effects on Galaxy Redshift Samples due to Target Selection
• VALES VI: ISM enrichment in star-forming galaxies up to z$\sim$0.2 using ${}^{12}$CO(1-0), ${}^{13}$CO(1-0) and C${}^{18}$O(1-0) line luminosity ratios
• Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1<z<0.35
• Galaxy And Mass Assembly (GAMA): Defining Passive Galaxy Samples and Searching for the UV Upturn
• Galaxy And Mass Assembly (GAMA): Self-Organizing Map Application on Nearby Galaxies
• TEGLIE: Transformer encoders as strong gravitational lens finders in KiDS
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• The detection of a massive chain of dark HI clouds in the GAMA G23 Field
• XXL-HSC: An updated catalogue of high-redshift ($z⩾3.5$) X-ray AGN in the XMM-XXL northern field. Constraints on the bright end of the soft logN-logS
• Cosmic Filaments from Cosmic Strings
• Connecting MeerKAT radio continuum properties to GAMA optical emission-line and WISE mid-infrared activity
• An optimised tiling pattern for multi-object spectroscopic surveys: application to the 4MOST survey
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
• Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
• Galaxy-scale gravitational lens candidates from the Hyper Suprime-Cam imaging survey and the Galaxy And Mass Assembly spectroscopic survey
• The SAMI Galaxy Survey: The contribution of different kinematic classes to the stellar mass function of nearby galaxies
• Pre-processing of Galaxies in the Early Stages of Cluster Formation in Abell 1882 at $z$=0.139
• The Loneliest Galaxies in the Universe: A GAMA and GalaxyZoo Study on Void Galaxy Morphology
• Interpreting Internal Consistency of DES Measurements
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• VEXAS: VISTA EXtension to Auxiliary Surveys -- Data Release 2: Machine-learning based classification of sources in the Southern Hemisphere
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• The eROSITA Final Equatorial Depth Survey (eFEDS): SDSS spectroscopic observations of X-ray sources
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Centrally concentrated molecular gas driving galactic-scale ionised gas outflows in star-forming galaxies
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at $z=$ 4.5-8.5
• Galaxy And Mass Assembly (GAMA): Stellar-to-Dynamical Mass Relation I. Constraining the Precision of Stellar Mass Estimates
• The central dark matter fraction of massive early-type galaxies
• Galaxy And Mass Assembly (GAMA) Survey: The Merging Potential of Brightest Group Galaxies
• Selection of powerful radio galaxies with machine learning
• Galaxy evolution in compact groups II. Witnessing the influence of major structures in their evolution
• Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
• On the patchy appearance of the circum-Galactic medium and the influence of foreground absorption
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• Intrinsic galaxy alignments in the KiDS-1000 bright sample: dependence on colour, luminosity, morphology, and galaxy scale
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• VEXAS: the VISTA EXtension to Auxiliary Surveys -- Data Release 1: the Southern Galactic Hemisphere
• The Observable Supernova Rate in Galaxy-Galaxy Lensing Systems with the TESS Satellite
• A robust two-parameter description of the stellar profile of elliptical galaxies
• The SAMI Galaxy Survey: Detection of Environmental Dependence of Galaxy Spin in Observations and Simulations Using Marked Correlation Functions
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• Halo shapes constrained from a pure sample of central galaxies in KiDS-1000
• Supersoft, luminous X-ray sources in galactic nuclei
• Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• VALES V: A kinematic analysis of the molecular gas content in $H$-ATLAS galaxies at $z\sim 0.03-0.35$ using ALMA
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• The infrared-radio relation in the local universe
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• A rising tide: Intrinsic alignments since the turn of the millennium
• Galaxy Properties Derived with Spectral Energy Distribution Fitting in the Hawaii-Hubble Deep Field-North
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• Shape noise and dispersion in precision weak lensing
• Deficit of Luminous and Normal Red Galaxies in Cosmic Voids
• Red riding on hood: Exploring how galaxy colour depends on environment
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Rejection criteria based on outliers in the KiDS photometric redshifts and PDF distributions derived by machine learning
• Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly$\alpha$ emitters and IGM transmission in the COSMOS field at $z\sim 5$
• The case for two-dimensional galaxy-galaxy lensing
• The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies
• Galaxy and Mass Assembly (GAMA): Low-redshift Quasars and Inactive Galaxies Have Similar Neighbors
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• Central star formation in an early-type galaxy I~Zw~81 in the Bootes void
• Galaxy And Mass Assembly (GAMA): $\mathbf{z}\sim 0$ Galaxy Luminosity Function down to $\mathbf{L}\sim 10^6{\mathbf{L}}_{\odot }$ via Clustering Based Redshift Inference
• XXL-HSC: Host properties of X-ray detected AGNs in XXL clusters
• Semi-supervised classification of stars, galaxies and quasars using K-means and random-forest approaches
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• The galaxy environment in GAMA G3C groups using the Kilo Degree Survey Data Release 3
• A new approach to finding galaxy groups using Markov Clustering
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• Demise of Faint Satellites around Isolated Early-type Galaxies
• A search for HI absorption in distant star-forming galaxies with ASKAP-FLASH -- I. Selection and analysis of the radio sample
• AMICO galaxy clusters in KiDS-1000: cosmological sample
• VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z\sim 0.15$ traced with VLT/MUSE
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• Compact groups of galaxies in GAMA -- Probing the densest minor systems at intermediate redshifts
• Panchromatic SED fitting codes and modelling techniques
• Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Deep Extragalactic VIsible Legacy Survey (DEVILS): DR1 Blended Spectra Search for Candidate Strong Gravitational Lenses
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Dust sub-millimetre emission in green valley galaxies
• Effect of redshift bin mismatch on cross correlation between DESI Legacy Imaging Survey and Planck CMB lensing potential
• Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors
• Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe
• The Jet Paths of Radio AGN and their Cluster Weather
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• Cosmic Insights from Galaxy Clusters: Exploring Magnification Bias on Sub-millimeter Galaxies
• Antarctic Survey Telescope 3-3: Overview, System Performance and Preliminary Observations at Yaoan, Yunnan
• On the Origin of the Strong Optical Variability of Emission-line Galaxies
• The intragroup light in KiDS+GAMA groups: A stacking analysis
• Cosmic magnification on high-redshift submillimeter galaxies
• Galaxy And Mass Assembly (GAMA): The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• 3D intrinsic shapes of quiescent galaxies in observations and simulations
• Identification of Anomalous E+A Galaxies in GAMA Using an Isolation Forest
• Methodological refinement of the submillimeter galaxy cross-correlation function measurements and their uncertainty estimation
• Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies
• Galaxy And Mass Assembly: A new approach to quantifying dust in galaxies
• Cooperative photometric redshift estimation
• Measuring Cosmic Density of Neutral Hydrogen via Stacking the DINGO-VLA Data
• The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. II. Sample Selection
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• CNN photometric redshifts in the SDSS at $r\le 20$
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Luminosity Function of Galaxies in Voids: A Modification Inspired by Excursion Set Theory
• Deep ASKAP EMU Survey of the GAMA23 field: Properties of radio sources
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• HI Gas and Star Formation in Major Galaxy Pairs from the FAST All-Sky HI Survey (FASHI)
• AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Hybrid-z: Enhancing Kilo-Degree Survey bright galaxy sample photometric redshifts with deep learning
• Galaxy And Mass Assembly: A Comparison between Galaxy-Galaxy Lens Searches in KiDS/GAMA
• Active galactic nuclei and gravitational redshifts
• Using a Neural Network Classifier to Select Galaxies with the Most Accurate Photometric Redshifts
• The gaseous natal environments of GPS and CSS sources with ASKAP -- FLASH
• xGASS: characterizing the slope and scatter of the stellar mass - angular momentum relation for nearby galaxies
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG