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The ALPINE-ALMA [CII] survey: Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6
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Lyman‐Break Galaxies at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z\gtrsim 4$ \end{document} and the Evolution of the Ultraviolet Luminosity Density at High Redshift
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AN EXPONENTIAL DECLINE AT THE BRIGHT END OF THE z = 6 GALAXY LUMINOSITY FUNCTION
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THE MAJOR AND MINOR GALAXY MERGER RATES AT z < 1.5
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PROBING THE DAWN OF GALAXIES AT z ∼ 9-12: NEW CONSTRAINTS FROM HUDF12/XDF AND CANDELS DATA
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PHYSICAL PROPERTIES OF SPECTROSCOPICALLY CONFIRMED GALAXIES AT z ⩾ 6. II. MORPHOLOGY OF THE REST-FRAME UV CONTINUUM AND Lyα EMISSION
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UV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST LEGACY FIELDS
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THE SIZES OF z ∼ 6–8 LENSED GALAXIES FROM THE HUBBLE FRONTIER FIELDS ABELL 2744 DATA
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CORRECTING THE z ∼ 8 GALAXY LUMINOSITY FUNCTION FOR GRAVITATIONAL LENSING MAGNIFICATION BIAS
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Candels Multi-Wavelength Catalogs: Source Detection and Photometry in the Goods-South Field
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MORPHOLOGIES OF ∼190,000 GALAXIES AT z = 0–10 REVEALED WITH HST LEGACY DATA. I. SIZE EVOLUTION
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STRUCTURE AND MORPHOLOGIES OF z ∼ 7-8 GALAXIES FROM ULTRA-DEEP WFC3/IR IMAGING OF THE HUBBLE ULTRA-DEEP FIELD
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THE EVOLUTION OF THE ULTRAVIOLET LUMINOSITY FUNCTION FROM z ∼ 0.75 TO z ∼ 2.5 USING HST ERS WFC3/UVIS OBSERVATIONS
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The Abundance of Star-Forming Galaxies in the Redshift Range 8.5-12: new Results from the 2012 Hubble Ultra deep Field Campaign
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A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10
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The rest-frame UV luminosity function at z ≃ 4: a significant contribution of AGNs to the bright end of the galaxy population
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The rapid transition from star formation to AGN-dominated rest-frame ultraviolet light at z ≃ 4
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Galaxy pairs in the Sloan Digital Sky Survey – VIII. The observational properties of post-merger galaxies
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The merger fraction of active and inactive galaxies in the local Universe through an improved non-parametric classification
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The galaxy UV luminosity function at z ≃ 2 –4; new results on faint-end slope and the evolution of luminosity density
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Non-parametric analysis of the rest-frame UV sizes and morphological disturbance amongst L * galaxies at 4 < z < 8
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The impact of strong gravitational lensing on observed Lyman-break galaxy numbers at 4 ≤ z ≤ 8 in the GOODS and the XDF blank fields
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Using galaxy pairs to probe star formation during major halo mergers
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A chronicle of galaxy mass assembly in the EAGLE simulation
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Unveiling the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope
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The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: the z = 9 luminosity function and further evidence for a smooth decline in ultraviolet luminosity density at z≥ 8
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Massive close pairs measure rapid galaxy assembly in mergers at high redshift
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Discovery of bright z ≃ 7 galaxies in the UltraVISTA survey : Bright z ≃ 7 galaxies from UltraVISTA
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Distributed Optimization and Statistical Learning via the Alternating Direction Method of Multipliers
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EVOLUTION OF STELLAR-TO-HALO MASS RATIO AT z = 0–7 IDENTIFIED BY CLUSTERING ANALYSIS WITH THE HUBBLE LEGACY IMAGING AND EARLY SUBARU/HYPER SUPRIME-CAM SURVEY DATA
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MORPHOLOGIES OF ∼190,000 GALAXIES AT z = 0–10 REVEALED WITH HST LEGACY DATA. II. EVOLUTION OF CLUMPY GALAXIES
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THE EVOLUTION OF THE GALAXY STELLAR MASS FUNCTION AT z = 4–8: A STEEPENING LOW-MASS-END SLOPE WITH INCREASING REDSHIFT
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RESOLVING THE DISCREPANCY OF GALAXY MERGER FRACTION MEASUREMENTS AT z ∼ 0–3
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New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency
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HST Imaging of the Brightest z ∼ 8–9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function
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PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions
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Bridging Star-forming Galaxy and AGN Ultraviolet Luminosity Functions at z = 4 with the SHELA Wide-field Survey
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LSST: From Science Drivers to Reference Design and Anticipated Data Products
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Observational Constraints on the Merger History of Galaxies since z ≈ 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields
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The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
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The Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field
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Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 ≤ z ≤ 7.0
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Automated Mining of the ALMA Archive in the COSMOS Field (A 3 COSMOS). II. Cold Molecular Gas Evolution out to Redshift 6
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Galaxy Merger Rates up to z ∼ 3 Using a Bayesian Deep Learning Model: A Major-merger Classifier Using IllustrisTNG Simulation Data
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Galaxy Stellar Mass Functions from z ∼ 10 to z ∼ 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time
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Pure Density Evolution of the Ultraviolet Quasar Luminosity Function at 2 ≲ z ≲ 6
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