Galaxy And Mass Assembly (GAMA): relations of bulges, discs and spheroids
arXiv:1607.01096 · doi:10.1093/mnras/stw1495
Abstract
We perform automated bulge + disc decomposition on a sample of 7500 galaxies from the Galaxy And Mass Assembly (GAMA) survey in the redshift range of 0.002z0.06 using SIGMA, a wrapper around GALFIT3. To achieve robust profile measurements we use a novel approach of repeatedly fitting the galaxies, varying the input parameters to sample a large fraction of the input parameter space. Using this method we reduce the catastrophic failure rate significantly and verify the confidence in the fit independently of . Additionally, using the median of the final fitting values and the 16 and 84 percentile produces more realistic error estimates than those provided by GALFIT, which are known to be underestimated. We use the results of our decompositions to analyse the stellar mass - half-light radius relations of bulges, discs and spheroids. We further investigate the association of components with a parent disc or elliptical relation to provide definite disc and spheroid relations. We conclude by comparing our local disc and spheroid to simulated data from EAGLE and high redshift data from CANDELS-UDS. We show the potential of using the mass-size relation to study galaxy evolution in both cases but caution that for a fair comparison all data sets need to be processed and analysed in the same manner.
arXiv comment33 pages, 14 + 7 Figures, MNRAS accepted
References in corpus (95)
- Stellar population synthesis at the resolution of 2003
- The Sloan Digital Sky Survey: Technical Summary
- The Dust Content and Opacity of Actively Star-Forming Galaxies
- The Seventh Data Release of the Sloan Digital Sky Survey
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- The Formation of Galactic Disks
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics
- Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since
- Astrophysics Source Code Library
- The size distribution of galaxies in the Sloan Digital Sky Survey
- The SINS survey: SINFONI Integral Field Spectroscopy of z ~ 2 Star-forming Galaxies
- Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
- zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
- Passively Evolving Early-type Galaxies at 1.4<z<2.5 in the Hubble Ultra Deep Field
- The Galactic disk mass function: reconciliation of the HST and nearby determinations
- The Growth of Massive Galaxies Since z=2
- Confirmation of the remarkable compactness of massive quiescent galaxies at z~2.3: early-type galaxies did not form in a simple monolithic collapse
- Galaxy And Mass Assembly: Stellar Mass Estimates
- A Catalog of Bulge+Disk Decompositions and Updated Photometry for 1.12 Million Galaxies in the Sloan Digital Sky Survey
- Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
- Structural Properties of Pseudo-Bulges, Classical Bulges and Elliptical Galaxies: an SDSS Perspective
- The Formation of Disk Galaxies
- Strong size evolution of the most massive galaxies since z~2
- The size evolution of galaxies since z~3: combining SDSS, GEMS and FIRES
- HST photometry of dwarf elliptical galaxies in Coma, and an explanation for the alleged structural dichotomy between dwarf and bright elliptical galaxies
- The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
- SINFONI Integral Field Spectroscopy of z~2 UV-selected Galaxies: Rotation Curves and Dynamical Evolution
- Size evolution of the most massive galaxies at 1.7<z<3 from GOODS NICMOS survey imaging
- Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations
- A Revised Parallel-Sequence Morphological Classification of Galaxies: Structure and Formation of S0 and Spheroidal Galaxies
- Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
- Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis (SIGMA)
- Evidence for Mature Bulges and an Inside-out Quenching Phase 3 Billion Years After the Big Bang
- Galaxy And Mass Assembly (GAMA): mass-size relations of z0.1 galaxies subdivided by Sérsic index, colour and morphology
- The Millennium Galaxy Catalogue: morphological classification and bimodality in the colour-concentration plane
- GEMS: Galaxy fitting catalogues and testing parametric galaxy fitting codes
- Imfit: A Fast, Flexible New Program for Astronomical Image Fitting
- Angular momentum and galaxy formation revisited
- Compact High-Redshift Galaxies Are the Cores of the Most Massive Present-Day Spheroids
- Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations
- The Hierarchical Origin of Galaxy Morphologies
- The Millennium Galaxy Catalogue: Bulge/Disc Decomposition of 10095 Nearby Galaxies
- Galaxy Size Evolution at High Redshift and Surface Brightness Selection Effects: Constraints from the Hubble Ultra Deep Field
- Discriminating Between the Physical Processes that Drive Spheroid Size Evolution
- The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history
- Size evolution of normal and compact galaxies in the EAGLE simulation
- BUDDA: A New Two-Dimensional Bulge/Disk Decomposition Code for Detailed Structural Analysis of Galaxies
- A catalogue of 2D photometric decompositions in the SDSS-DR7 spectroscopic main galaxy sample: preferred models and systematics
- Galaxy And Mass Assembly (GAMA): Spectroscopic analysis
- Image Decomposition of Barred Galaxies and AGN Hosts
- Dissecting the size evolution of elliptical galaxies since z~1: puffing up vs minor merging scenarios
- Galaxy And Mass Assembly (GAMA): Accurate Panchromatic Photometry from Optical Priors using LAMBDAR
- The Morphologies of Massive Galaxies at 1<z<3 in the CANDELS-UDS Field: Compact Bulges, and the Rise and Fall of Massive Disks
- Curvature in the scaling relations of early-type galaxies
- Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget
- Galaxy Zoo: Observing Secular Evolution Through Bars
- Early type galaxies have been the predominant morphological class for massive galaxies since only z~1
- E/S0 Galaxies on the Blue Color-Stellar Mass Sequence at z=0: Fading Mergers or Future Spirals?
- The Redshift and Mass Dependence on the Formation of The Hubble Sequence at z>1 from CANDELS/UDS
- The Kormendy relation of massive elliptical galaxies at z~1.5. Evidence for size evolution ?
- Astrophysically Motivated Bulge-Disk Decompositions of SDSS Galaxies
- Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors
- The Dawes Review 1: Kinematic studies of star-forming galaxies across cosmic time
- The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes
- High star formation rates as the origin of turbulence in early and modern disk galaxies
- Galaxy And Mass Assembly (GAMA): The input catalogue and star-galaxy separation
- Galaxy and Mass Assembly (GAMA): FUV, NUV, ugrizYJHK Petrosian, Kron and Sèrsic photometry
- Scaling Relations of Star-Forming Regions: from kpc-size clumps to HII regions
- Deconstructing the Galaxy Stellar Mass Function with UKIDSS and CANDELS: the Impact of Colour, Structure and Environment
- Hyper-Fit: Fitting Linear Models to Multidimensional Data with Multivariate Gaussian Uncertainties
- Galaxy And Mass Assembly (GAMA): the Stellar Mass Budget by Galaxy Type
- A review of elliptical and disc galaxy structure, and modern scaling laws
- Mid-Infrared Galaxy Morphology from the Spitzer Survey of Stellar Structure in Galaxies (S^4G): The Imprint of the de Vaucouleurs Revised Hubble-Sandage Classification System at 3.6 microns
- Evidence of major dry mergers at M* > 2 x 10^11 Msun from curvature in early-type galaxy scaling relations?
- Keck-I MOSFIRE spectroscopy of compact star-forming galaxies at z2: High velocity dispersions in progenitors of compact quiescent galaxies
- Hiding in plain sight: An abundance of compact massive spheroids in the local Universe
- The Sizes of Candidate Galaxies: confirmation of the bright CANDELS sample and relation with luminosity and mass
- Two-phase galaxy evolution: the cosmic star-formation histories of spheroids and discs
- Mass assembly of galaxies: Smooth accretion versus mergers
- Galaxy And Mass Assembly (GAMA): Curation and reanalysis of 16.6k redshifts in the G10/COSMOS region
- The Millennium Galaxy Catalogue: Exploring the Color-Concentration Bimodality via Bulge-Disc Decomposition
- Insights on the Formation, Evolution, and Activity of Massive Galaxies From Ultra-Compact and Disky Galaxies at z=2-3
- The effects of dust on the derived photometric parameters of disks and bulges in spiral galaxies
- The Decomposed Bulge and Disk Size-Mass Relations of Massive Galaxies at 1<z<3 in CANDELS
- Gas Mass Fractions and Star Formation in Blue-Sequence E/S0 Galaxies
- Two-Phase Galaxy Formation
- The effects of dust on the photometric parameters of decomposed disks and bulges
- The Formation of Bulges, Discs and Two Component Galaxies in the CANDELS Survey at z < 3
- Galaxy And Mass Assembly (GAMA): Understanding the wavelength dependence of galaxy structure with bulge-disc decompositions
- The evolution of disc galaxies with and without classical bulges since z~1
- The signature of dissipation in the mass-size relation: are bulges simply spheroids wrapped in a disc?
- The zCOSMOS Redshift Survey: evolution of the light in bulges and discs since z~0.8
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- The diverse nature and formation paths of slow rotator galaxies in the EAGLE simulations
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- Figuring Out Gas & Galaxies In Enzo (FOGGIE). IV. The Stochasticity of Ram Pressure Stripping in Galactic Halos
- Evolution of galactic magnetic fields
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- The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
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- The structural properties of classical bulges and discs from z~2
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