Structural Parameters of Galaxies in CANDELS
arXiv:1211.6954 · doi:10.1088/0067-0049/203/2/24
Abstract
We present global structural parameter measurements of 109,533 unique, H_F160W-selected objects from the CANDELS multi-cycle treasury program. Sersic model fits for these objects are produced with GALFIT in all available near-infrared filters (H_F160W, J_F125W and, for a subset, Y_F105W). The parameters of the best-fitting Sersic models (total magnitude, half-light radius, Sersic index, axis ratio, and position angle) are made public, along with newly constructed point spread functions for each field and filter. Random uncertainties in the measured parameters are estimated for each individual object based on a comparison between multiple, independent measurements of the same set of objects. To quantify systematic uncertainties we create a mosaic with simulated galaxy images with a realistic distribution of input parameters and then process and analyze the mosaic in an identical manner as the real data. We find that accurate and precise measurements -- to 10% or better -- of all structural parameters can typically be obtained for galaxies with H_F160W < 23, with comparable fidelity for basic size and shape measurements for galaxies to H_F160W ~ 24.5.
public data release of structural parameters from CANDELS WFC3 data: http://www.mpia-hd.mpg.de/homes/vdwel/candels.html
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- SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-m-selected sub-millimeter galaxies
- An ALMA view of 11 Dusty Star Forming Galaxies at the peak of Cosmic Star Formation History
- The effect of environment on star formation activity and morphology at 0.5 < z < 2.5 in CANDELS
- High Redshift Massive Quiescent Galaxies are as Flat as Star Forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST
- Identification and Characterization of a Large Sample of Distant Active Dwarf Galaxies in XMM-SERVS
- The massive dark halo of the compact, early-type galaxy NGC 1281
- Differences in the structural properties and star-formation rates of field and cluster galaxies at z~1
- Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
- The discrepancy between dynamical and stellar masses in massive compact galaxies traces non-homology
- Rest-Frame Near-Infrared Radial Light Profiles up to z=3 from JWST/NIRCam: Wavelength Dependence of the Sérsic Index
- Similarities and uniqueness of Ly emitters among star-forming galaxies at z=2.5
- The MOSDEF-LRIS Survey: Connection between Galactic-scale Outflows and the Properties of ~2 star-forming Galaxies
- DAWN JWST Archive: Morphology from profile fitting of over 340 000 galaxies in major fields
- Spatially resolved mass-metallicity relation at z~0.26 from the MUSE-Wide Survey
- The structure of massive quiescent galaxies at z~3 in the CANDELS-COSMOS field
- Dust attenuation, dust content and geometry of star-forming galaxies
- Deep Extragalactic VIsible Legacy Survey (DEVILS): The emergence of bulges and decline of disk growth since
- Measuring the average molecular gas content of star-forming galaxies at
- Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS
- The star formation history and the nature of the mass-metallicity relation of passive galaxies at 1.0<z<1.4 from VANDELS
- The role of gas kinematics in setting metallicity gradients at high redshift
- CANDELS Meets GSWLC: Evolution of the Relationship Between Morphology and Star Formation Since z = 2
- The cosmic epoch dependence of environmental effects on size evolution of red-sequence early-type galaxies
- On the detectability of strong lensing in near-infrared surveys
- An Extensive Photometric Catalog of CALIFA Galaxies
- Connecting Galactic Outflows and Star Formation: Inferences from H-alpha Maps and Absorption Line Spectroscopy at 1 < z < 1.5
- Measuring alignments between galaxies and the cosmic web at using IGM tomography
- Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic Systems
- Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
- K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at -
- On the limits of measuring the bulge and disk properties of local and high-redshift massive galaxies
- Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since
- Physical properties of compact star-forming galaxies at
- Compact star-forming galaxies preferentially quenched to become PSBs in clusters
- Deep learning for studies of galaxy morphology
- Euclid preparation. XXX. Performance assessment of the NISP Red-Grism through spectroscopic simulations for the Wide and Deep surveys
- Witnessing an extreme, highly efficient galaxy formation mode with resolved Ly and LyC emission
- JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
- The principle of maximum entropy explains the cores observed in the mass distribution of dwarf galaxies
- Gaia Data Release 3: Surface brightness profiles of galaxies and host galaxies of quasars
- Listening to galaxies tuning at z ~ 2.5 - 3.0: The first strikes of the Hubble fork
- Analysis of the galaxy size versus stellar mass relation
- Unveiling Sizes of Compact AGN Hosts with ALMA
- On the Impact of Inclination-Dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
- Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey
- Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies
- The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalog
- The mass dependence of structure, star formation rate, and mass assembly mode at 0.5<z< 2.5
- Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
- Stellar systems following the luminosity law. III. Photometric, intrinsic, and dynamical properties for all Sérsic indices
- Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
- Molecular gas in distant brightest cluster galaxies
- Stellar systems following the luminosity law. IV. The total energy and the central concentration of galaxies
- The Velocity Dispersion Function for Massive Quiescent and Star-Forming Galaxies at 0.6 z 1.0
- The MOSDEF Survey: Stellar Continuum Spectra and Star Formation Histories of Active, Transitional, and Quiescent Galaxies at 1.4\lowercase{z}2.6
- Projected distances to host galaxy reduce SNIa dispersion
- SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies
- Searching for the connection between ionizing-photon escape and the surface density of star formation at z~3
- Structures, stellar population properties, AGN fractions, and environments of massive compact galaxies at in 3D--{\it HST}/CANDELS
- MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
- Bayesian fitting of multi-Gaussian expansion models to galaxy images
- Structural analysis of massive galaxies using HST deep imaging at z < 0.5
- Environments of red nuggets at z~0.7 from the VIPERS survey
- Multiwavelength Bulge-Disk Decomposition for the Galaxy M81 (NGC 3031). I. Morphology
- FIGS: Spectral fitting constraints on the star formation history of massive galaxies since Cosmic Noon
- Evolution of the Sérsic Index up to z=2.5 from JWST and HST
- The Role of Bulge Formation in the Homogenization of Stellar Populations at as revealed by Internal Color Dispersion in CANDELS
- GALFIT-ing AGN Host Galaxies in COSMOS: HST vs. Subaru
- Validation of PSF Models for HST and Other Space-Based Observations
- Probing galaxy evolution from to through galaxy scaling relations in three L-Galaxies flavours
- The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3
- UV-Bright Star-Forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 z 1
- A galactic outflow traced by its extended Mg II emission out to a kpc radius in the Hubble Ultra Deep Field with MUSE
- Galaxy Ellipticity Measurements in the Near-Infrared for Weak Lensing
- Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
- Galaxy populations in the most distant SPT-SZ clusters -- II. Galaxy structural properties in massive clusters at 1.4<z<1.7
- The extragalactic -ray background: imprints from the physical properties and evolution of star-forming galaxy populations
- Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies at z ~ 1.4
- A new fitting concept for the robust determination of Sérsic model parameters
- PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z<2.5
- Using Multiple Emission Line Ratios to Constrain the Slope of the Dust Attenuation Law
- The PSF Smoothing Effect on Concentration-Related Parameters of High Redshift Galaxies in HST and JWST
- The SCUBA-2 Cosmology Legacy Survey: The EGS deep field -- III. The evolution of faint submillimeter galaxies at
- The Isophotal Structure of Star-forming Galaxies at in CANDELS: Implications for the Evolution of Galaxy Structure
- HELLO project: High- Evolution of Large and Luminous Objects
- NOEMA: A first kpc resolution study of a main sequence barred galaxy channeling gas into a growing bulge
- The Dwarf Galaxy Population at : A Catalog of Emission Lines and Redshifts from Deep Keck Observations
- Identifying Lyα emitter candidates with Random Forest: learning from galaxies in CANDELS survey
- Anomalously Narrow Linewidths of Compact Massive Star-Forming Galaxies at z~2.3: A Possible Inclination Bias in the Size-Mass Plane
- The Chandra Deep Field South as a test case for Global Multi Conjugate Adaptive Optics
- CONGRuENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra). I. A predictive model for galactic non-thermal emission
- A subarcsecond near-infrared view of massive galaxies at z > 1 with Gemini Multiconjugate Adaptive Optics
- The abundance of massive compact galaxies at in 3D-HST/CANDELS
- Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
- Properties of galaxies at the faint end of the H luminosity function at
- Morphology and structure of BzK-selected galaxies at z~2 in the CANDELS-COSMOS field
- Kinematic scaling relations of disc galaxies from ionised gas at and their connection with dark matter haloes
- Discovery of faint double-peak Halpha emission in the halo of low redshift galaxies
- Photometric properties of classical bulge and pseudo-bulge galaxies at
- Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since
- Central star formation in double-peak gas rich radio galaxies
- A Large Massive Quiescent Galaxy Sample at z~1.2
- The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
- A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn
- The VANDELS Survey: Star formation and quenching in two over-densities at 3 < z < 4
- A Ringed Dwarf LINER 1 Galaxy Hosting an Intermediate-mass Black Hole with Large-scale Rotation-like Hα Emission
- The Intrinsic Flattening of Galaxy Disks
- Improved SED-Fitting Assumptions Result in Inside-Out Quenching at and Quenching at All Radii Simultaneously at
- Exploring high-z galaxies with the E-ELT
- The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
- Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
- The MOSDEF Survey: A New View of a Remarkable z=1.89 Merger
- Automatic morphological classification of galaxies: convolutional autoencoder and bagging-based multiclustering model
- A Bending in the Size-mass Relation of Star-forming Galaxies across at a Critical Stellar Mass of Revealed by JWST
- Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn
- CONGRuENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra). II. Population-level correlations between galactic infrared, radio, and γ-ray emission
- The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
- Probing the influence of the protocluster environment on galaxy morphology at z = 2.23
- Dynamical properties and star formation history of a low-mass quenched galaxy at Cosmic Noon
- Recent star formation in 0.5<z<1.5 quiescent galaxies
- Reconstructing the Assembly of Massive Galaxies. III: Quiescent Galaxies Loose Angular Momentum as They Evolve in a Mass-dependent Fashion
- Morphology and structure of extremely red objects at in the CANDELS-COSMOS field
- Structural and morphological properties of ultraluminous infrared galaxies at
- Physically motivated fit to mass surface density profiles observed in galaxies
- The Compact Star-Forming Galaxies at in 3D-HST/CANDELS: AGN and Non-AGN Physical Properties
- Separating the Optical to Near-Infrared Light of AGN and Their Host Galaxies
- Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
- Compact star forming galaxies as the progenitors of compact quiescent galaxies: clustering result
- Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScience
- The multiwavelength structure of post-starburst galaxies at 0.5 < z < 3 with JWST PRIMER: compact morphologies and residual disturbances
- Lack of influence of the environment in the earliest stages of massive galaxy formation