Galapagos-2/Galfitm/GAMA -- multi-wavelength measurement of galaxy structure: separating the properties of spheroid and disk components in modern surveys
arXiv:2204.05907 · doi:10.1051/0004-6361/202142935
Abstract
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 fitting of large samples of galaxies in future surveys. We release both the code and the fit results to 234,239 objects from the DR3 of the Gama survey, a sample significantly deeper than previous works. We use stringent tests on both simulated and real data, as well as comparison to public catalogues to evaluate the advantages of using multi-band over single-band data. We show that multi-band fitting using Galfitm provides significant advantages when trying to decompose galaxies into their individual constituents, as more data are being used, by effectively being able to use the colour information buried in the individual exposures to its advantage. Using simulated data, we find that multi-band fitting significantly reduces the deviations from real parameter values, allows component sizes and Sérsic indices to be recovered more accurately, and, by design, constrains the band-to-band variations of these parameters to more physical values. On both simulated and real data, we confirm that the SEDs of the 2 main components can be recovered to fainter magnitudes compared to using single-band fitting, which tends to recover disks and bulges to - on average - have identical SEDs when the galaxies become too faint, instead of the different SEDs they truly have. By comparing our results to those provided by other fitting codes, we confirm that they agree in general, but measurement errors can be significantly reduced by using the multi-band tools developed by the MegaMorph project. We conclude that the multi-band fitting employed by Galapagos-2 and Galfitm significantly improves the accuracy of structural galaxy parameters and enables much larger samples to be be used in a scientific analysis.
arXiv comment50 pages, 30 figures, accepted for publication in A&A
References in corpus (68)
- The Sloan Digital Sky Survey: Technical Summary
- Detailed Structural Decomposition of Galaxy Images
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- 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
- The Cosmic Evolution Survey (COSMOS) -- Overview
- Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models
- The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
- Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey
- The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
- CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation
- The size distribution of galaxies in the Sloan Digital Sky Survey
- Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
- The Relationship Between Stellar Light Distributions of Galaxies and their Formation Histories
- A New Non-Parametric Approach to Galaxy Morphological Classification
- A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes
- A Catalog of Bulge+Disk Decompositions and Updated Photometry for 1.12 Million Galaxies in the Sloan Digital Sky Survey
- The Frontier Fields: Survey Design
- Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
- The COMBO-17 Survey: Evolution of the Galaxy Luminosity Function from 25,000 Galaxies with 0.2<z<1.2
- GEMS: Galaxy Evolution from Morphologies and SEDs
- Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis (SIGMA)
- GEMS: Galaxy fitting catalogues and testing parametric galaxy fitting codes
- Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3
- A catalog of bulge, disk, and total stellar mass estimates for the Sloan Digital Sky Survey
- Evidence for a New Elliptical-Galaxy Paradigm: Sersic and Core Galaxies
- The Millennium Galaxy Catalogue: Bulge/Disc Decomposition of 10095 Nearby Galaxies
- The Millennium Galaxy Catalogue: the B-band attenuation of bulge and disc light and the implied cosmic dust and stellar mass densities
- MegaMorph - multi-wavelength measurement of galaxy structure: complete Sérsic profile information from modern surveys
- Modelling the spectral energy distribution of galaxies. III. Attenuation of stellar light in spiral galaxies
- A catalogue of 2D photometric decompositions in the SDSS-DR7 spectroscopic main galaxy sample: preferred models and systematics
- Modelling the spectral energy distribution of galaxies. V. The dust and PAH emission SEDs of disk galaxies
- ProFound: Source Extraction and Application to Modern Survey Data
- Ages of galaxy bulges and disks from optical and near-infrared colors
- Evolution of Disk Galaxies in the GOODS-South Field: Number Densities and Size Distribution
- The ALHAMBRA Project: A large area multi medium-band optical and NIR photometric survey
- Astrophysically Motivated Bulge-Disk Decompositions of SDSS Galaxies
- Galaxy And Mass Assembly (GAMA): relations of bulges, discs and spheroids
- MegaMorph -- multi-wavelength measurement of galaxy structure: Sérsic profile fits to galaxies near and far
- ProFit: Bayesian Profile Fitting of Galaxy Images
- The SAMI Galaxy Survey: the third and final data release
- Galaxy And Mass Assembly (GAMA): the wavelength-dependent sizes and profiles of galaxies revealed by MegaMorph
- Galaxy Zoo: Secular evolution of barred galaxies from structural decomposition of multi-band images
- Mass assembly and morphological transformations since from CANDELS
- SDSS-IV MaNGA PyMorph Photometric and Deep Learning Morphological Catalogs and implications for bulge properties and stellar angular momentum
- Dark Matter and Stellar Mass in the Luminous Regions of Disk Galaxies
- Extending the evolution of the stellar mass-size relation at to low stellar mass galaxies from HFF and CANDELS
- First discoveries of z~6 quasars with the Kilo Degree Survey and VISTA Kilo-Degree Infrared Galaxy survey
- Modelling the spectral energy distribution of galaxies. IV Correcting apparent disk scalelengths and central surface brightnesses for the effect of dust at optical and near-infrared wavelengths
- The Bulge-Disk Decomposed Evolution of Massive Galaxies at 1<z<3 in CANDELS
- A catalog of polychromatic bulge-disk decompositions of ~ 17.600 galaxies in CANDELS
- Simulations of single and two-component galaxy decompositions for spectroscopically selected galaxies from the Sloan Digital Sky Survey
- PyMorph: Automated Galaxy Structural Parameter Estimation using Python
- FitSKIRT: genetic algorithms to automatically fit dusty galaxies with a Monte Carlo radiative transfer code
- The Decomposed Bulge and Disk Size-Mass Relations of Massive Galaxies at 1<z<3 in CANDELS
- Dissecting the Red Sequence: The Bulge and Disc Colours of Early-Type Galaxies in the Coma Cluster
- MegaMorph -- multi-wavelength measurement of galaxy structure: physically meaningful bulge-disc decomposition of galaxies near and far
- SDSS-IV MaNGA: Bulge-Disc Decomposition of IFU Datacubes (BUDDI)
- The effects of dust on the photometric parameters of decomposed disks and bulges
- Galaxy And Mass Assembly (GAMA): Understanding the wavelength dependence of galaxy structure with bulge-disc decompositions
- Galaxy And Mass Assembly (GAMA): the wavelength dependence of galaxy structure versus redshift and luminosity
- Colours of Bulges and Discs within Galaxy Clusters and the Signature of Disc Fading on Infall
- Dust emission profiles of DustPedia galaxies
- Galaxy Zoo: Finding offset discs and bars in SDSS galaxies
- Galaxy And Mass Assembly (GAMA): Galaxy colour gradients versus colour, structure and luminosity
- Formation of S0s in extreme environments II: the star-formation histories of bulges, discs and lenses
- A radiative transfer model for the spiral galaxy M33
- Estimating Sky Level
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- Euclid preparation XXVI. The Euclid Morphology Challenge. Towards structural parameters for billions of galaxies
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- Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey
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- The miniJPAS Survey: The radial distribution of star formation rates in faint X-ray active galactic nuclei
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