The DEEP Groth Strip Survey II. Hubble Space Telescope Structural Parameters of Galaxies in the Groth Strip

Abstract

The quantitative morphological classification of distant galaxies is essential to the understanding of the evolution of galaxies over the history of the Universe. This paper presents Hubble Space Telescope WFPC2 F606W and F814W photometric structural parameters for 7450 galaxies in the ``Groth Strip.'' These parameters are based on a two-dimensional bulge+disk surface brightness model and were obtained using an automated reduction and analysis pipeline described in detail here. A first set of fits was performed separately in each bandpass, and a second set of fits was performed simultaneously on both bandpasses. The information produced by these two types of fits can be used to explore different science goals. Systematic and random fitting errors in all structural parameters as well as bulge and disk colors are carefully characterized through extensive sets of simulations. The results of these simulations are given in catalogs similar to the real science catalogs so that both real and simulated measurements can be sampled according to the same selection criteria to show biases and errors in the science data subset of interest. The effects of asymmetric structures on the recovered bulge+disk fitting parameters are also explored through simulations. The full multidimensional photometric survey selection function of the Groth Strip is also computed. This selection function, coupled to bias maps from simulations, provides a complete and objective reproduction of the observational limits, and these limits can be applied to theoretical predictions from galaxy evolution models for direct comparisons with the data.

22 pages+16 PNG/JPEG figures, ApJ Supplements accepted. Full resolution paper+figures at http://deep.ucolick.org/publications.html . Tables 2 and 3 available upon publication of the redshift catalogue (Phillips et al. in prep.). Observed quantities available through interactive database at http://saci.ucolick.org

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• Discovery of extremely low-metallicity circumgalactic gas at $z=0.5$ toward Q0454-220
• The dust effects on galaxy scaling relations
• Bulges of disk galaxies at intermediate redshifts. I. Samples with and without bulges in the Groth Strip Survey
• 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
• The peculiar galaxy Mkn 298 revisited through integral field spectroscopy
• CG J1720-67.8: A Detailed Analysis of Optical and Infrared Properties of a New Ultracompact Group of Galaxies
• Growth of disc-like pseudo-bulges in SDSS DR7 since z = 0.1
• A new fitting concept for the robust determination of Sérsic model parameters
• Smaller stellar disc scale lengths in rich environments
• Probing the circumgalactic medium of active galactic nuclei with background quasars
• The PSF Smoothing Effect on Concentration-Related Parameters of High Redshift Galaxies in HST and JWST
• X-ray emission properties of galaxies in Abell 3128
• Decomposing galaxies with BANG: an automated morpho-kinematical decomposition of the SDSS-DR17 MaNGA survey
• On the Structure of the AGN Torus through the Fraction of Optically-Selected Type 1 AGNs
• SDSS J121811.0+465501.2: a new Low Surface Brightness Galaxy with low metallicity
• The morphologies and masses of extremely red galaxies in the Groth Strip survey
• Dust effects on the derived Sersic indexes of disks and bulges in spiral galaxies
• Global Optimization methods for Gravitational Lens Systems with Regularized Sources
• Local galaxies with compact cores as the possible descendants of massive compact quiescent galaxies at high redshift
• Ground-based image deconvolution with Swin Transformer UNet
• Powerful Radio Emission From Low-mass Supermassive Black Holes Favors Disk-like Bulges
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• How the spectral energy distribution and galaxy morphology constrain each other, with application to morphological selection using galaxy colours
• Structure and mass distribution of spiral galaxies at intermediate redshifts
• Low-mass and High-mass Supermassive Blackholes In Radio-Loud AGNs Are Spun-up in Different Evolution Paths
• CATS: Optical to Near-Infrared Colors of the Bulge and Disk of Two z=0.7 Galaxies Using HST and Keck Laser Adaptive Optics Imaging
• On the scaling relations of bulges and early-type galaxies
• Maximally informed Bayesian modelling of disc galaxies
• The link between galaxy structure properties and star formation in local galaxies
• Non-parametric decompositions of disk galaxies in S${}^4$G using DiskFit
• SDSS-IV MaNGA: Stellar rotational support in disk galaxies vs. central surface density and stellar population age
• The z=0.8 precursors of today's bulges
• Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies
• Recovering 3D structural properties of galaxies from SDSS-like photometry
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Morphologies for DECaLS Galaxies through a combination of non-parametric indices and machine learning methods: A comprehensive catalog using the Galaxy Morphology Extractor (galmex) code
• Star Formation Properties in Barred Galaxies (SFB). II. NGC 2903 and NGC 7080