Observations of the Initial Formation and Evolution of Spiral galaxies at $1<z<3$ in the CANDELS fields

Abstract

Many aspects concerning the formation of spiral and disc galaxies remain unresolved, despite their discovery and detailed study over the past $150$ years. As such, we present the results of an observational search for proto-spiral galaxies and their earliest formation, including the discovery of a significant population of spiral-like and clumpy galaxies at $z>1$ in deep \textit{Hubble Space Telescope} CANDELS imaging. We carry out a detailed analysis of this population, characterising their number density evolution, masses, star formation rates and sizes. Overall, we find a surprisingly high overall number density of massive $M_{\ast }>10^{10}{\mathrm{M}}_{\odot }$ spiral-like galaxies (including clumpy spirals) at $z>1$ of $0.18\mathrm{per}{\mathrm{arcmin}}^{-2}$. We measure and characterise the decline in the number of these systems at higher redshift using simulations to correct for redshift effects in identifications, finding that the true fraction of spiral-like galaxies grows at lower redshifts as $\sim$ $(1+z{)}^{-1.1}$. This is such that the absolute numbers of spirals increases by a factor of $\sim 10$ between $z=2.5$ and $z=0.5$. We also demonstrate that these spiral-like systems have large sizes at $z>2$, and high star formation rates, above the main-sequence, These galaxies represent a major mode of galaxy formation in the early universe, perhaps driven by the spiral structure itself. We finally discuss the origin of these systems, including their likely formation through gas accretion and minor mergers, but conclude that major mergers are an unlikely cause.

arXiv commentMNRAS accepted, 18 pages

References in corpus (64)

• Stellar population synthesis at the resolution of 2003
• Star Formation in Galaxies Along the Hubble Sequence
• Detailed Structural Decomposition of Galaxy Images
• 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
• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey
• The Star-formation Mass Sequence out to z=2.5
• The Relationship Between Stellar Light Distributions of Galaxies and their Formation Histories
• Structural Parameters of Galaxies in CANDELS
• CANDELS Multi-wavelength Catalogs: Source Detection and Photometry in the GOODS-South Field
• A Direct Measurement of Major Galaxy Mergers at z < 3
• The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies
• The rapid formation a large rotating disk galaxy three billion years after the Big Bang
• Size evolution of the most massive galaxies at 1.7<z<3 from GOODS NICMOS survey imaging
• Star Formation in NGC5194 (M51a): The Panchromatic View from GALEX to Spitzer
• Structural and Photometric Classification of Galaxies - I. Calibration Based on a Nearby Galaxy Sample
• The Kiloparsec-Scale Kinematics of High-Redshift Star-Forming Galaxies
• A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation
• Star Formation from Galaxies to Globules
• CANDELS Multiwavelength catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-Deep Survey Field
• The mass evolution of the first galaxies: stellar mass functions and star formation rates at $4<z<7$ in the CANDELS GOODS-South field
• The evolution of the dust and gas content in galaxies
• Stellar Populations in Ten Clump-Cluster Galaxies of the Ultra Deep Field
• Giant Molecular Clouds in M33 - I. BIMA All Disk Survey
• Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3
• The Luminosity, Stellar Mass, and Number Density Evolution of Field Galaxies of Known Morphology from z = 0.5 - 3
• MegaMorph - multi-wavelength measurement of galaxy structure: complete Sérsic profile information from modern surveys
• The Fundamental Properties of Galaxies and a New Galaxy Classification System
• Clumpy Galaxies in GOODS and GEMS: Massive Analogs of Local Dwarf Irregulars
• Simulations of the grand design galaxy M51: a case study for analysing tidally induced spiral structure
• Galaxy Morphologies in the Hubble Ultra Deep Field: Dominance of Linear Structures at the Detection Limit
• The structures and total (minor + major) merger histories of massive galaxies up to z = 3 in the HST GOODS NICMOS Survey: A possible solution to the size evolution problem
• GALAPAGOS: From Pixels to Parameters
• The Morphologies of Massive Galaxies at 1<z<3 in the CANDELS-UDS Field: Compact Bulges, and the Rise and Fall of Massive Disks
• Early type galaxies have been the predominant morphological class for massive galaxies since only z~1
• The Redshift and Mass Dependence on the Formation of The Hubble Sequence at z>1 from CANDELS/UDS
• CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
• Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type
• MegaMorph -- multi-wavelength measurement of galaxy structure: Sérsic profile fits to galaxies near and far
• Observing the Formation of the Hubble Sequence in the Great Observatories Origins Deep Survey
• Deconstructing the Galaxy Stellar Mass Function with UKIDSS and CANDELS: the Impact of Colour, Structure and Environment
• Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELS
• Mass assembly and morphological transformations since $z\sim 3$ from CANDELS
• Grand Design and Flocculent Spirals in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
• Galaxy Light Concentration. I. Index stability and the connection with galaxy structure, dynamics, and supermassive black holes
• Galaxy Populations and Evolution in Clusters II: Defining Cluster Populations
• Age distributions of star clusters in spiral and barred galaxies as a test for theories of spiral structure
• High Velocity Dispersion in A Rare Grand Design Spiral Galaxy at Redshift z=2.18
• The Bulge-Disk Decomposed Evolution of Massive Galaxies at 1<z<3 in CANDELS
• Attenuation caused by a distant Isothermal Turbulent Screen
• Simulations of Normal Spiral Galaxies
• The Onset of Spiral Structure in the Universe
• The Effect of Spiral Arms on Star Formation in the Galaxy
• MegaMorph -- multi-wavelength measurement of galaxy structure: physically meaningful bulge-disc decomposition of galaxies near and far
• FERENGI: Redshifting galaxies from SDSS to GEMS, STAGES and COSMOS
• The Formation of Bulges, Discs and Two Component Galaxies in the CANDELS Survey at z < 3
• Optical and Near-Infrared Spectroscopy of a High-Redshift, Hard X-ray Emitting Spiral Galaxy
• Galaxy Zoo: star-formation versus spiral arm number
• Unbiased Differential Size Evolution and the Inside-Out Growth of Galaxies in the Deep CANDELS GOODS Fields at $1\le z\le 7$
• The Evolution of Galaxies at Constant Number Density: A Less Biased View of Star Formation, Quenching, and Structural Formation
• Galaxy Zoo: constraining the origin of spiral arms
• Surface Brightness Evolution of Galaxies in the CANDELS GOODS Fields up to $z\sim 6$: High-z Galaxies are Unique or Remain Undetected
• Stellar populations, stellar masses and the formation of galaxy bulges and discs at $z<3$ in CANDELS

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• The rapid onset of stellar bars in the baryon-dominated centers of disk galaxies
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• A grand-design spiral galaxy 1.5 billion years after the Big Bang with JWST
• NOEMA${}^{3D}$: A first kpc resolution study of a $z\sim 1.5$ main sequence barred galaxy channeling gas into a growing bulge
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