Size evolution of the most massive galaxies at 1.7<z<3 from GOODS NICMOS survey imaging
arXiv:0807.4141 · doi:10.1086/592836
Abstract
We measure the sizes of 82 massive (M>10^11 M_sun) galaxies at 1.7<z<3 utilizing deep HST NICMOS data taken in the GOODS North and South fields. Our sample is almost an order of magnitude larger than previous studies at these redshifts, providing the first statistical study of massive galaxy sizes at z>2, confirming the extreme compactness of these galaxies. We split our sample into disk-like (n<2) and spheroid-like (n>2) galaxies based on their Sersic indices, and find that at a given stellar mass disk-like galaxies at z~2.3 are a factor of 2.6+/-0.3 smaller than present day equal mass systems, and spheroid-like galaxies at the same redshifts are 4.3+/-0.7 smaller than comparatively massive elliptical galaxies today. At z>2 our results are compatible with both a leveling off, or a mild evolution in size. Furthermore, the high density (~2x10^10 M_sun kpc^-3) of massive galaxies at these redshifts, which are similar to present day globular clusters, possibly makes any further evolution in sizes beyond z=3 unlikely.
arXiv comment5 pages, 2 figures, 2 tables, accepted by ApJ Letters, minor changes added to match the accepted version
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- Compactness of Cold Gas in High-Redshift Galaxies
- An Extensive Photometric Catalog of CALIFA Galaxies
- The role of major mergers in the size growth of intermediate-mass spheroids
- Exploring the progenitors of brightest cluster galaxies at z~2
- The Structures of Distant Galaxies V: The Evolution of Galaxy Structure in Stellar Mass at z < 1
- Characterizing the satellites of massive galaxies up to z~2: young populations to build the outskirts of nearby massive galaxies
- A comparison of the most massive quiescent galaxies from to the present: slow evolution in size, and spheroid-dominated
- On the limits of measuring the bulge and disk properties of local and high-redshift massive galaxies
- Compact Quiescent Galaxies at Intermediate Redshifts
- Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
- Physical properties of compact star-forming galaxies at
- Listening to galaxies tuning at z ~ 2.5 - 3.0: The first strikes of the Hubble fork
- The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
- Color gradients reflect an inside-out growth in early-type galaxies of the cluster MACS J1206.2-0847
- HST F160W Imaging of Very Massive Galaxies at : Diversity of Structures and the Effect of Close Pairs on Number Density Estimates
- Modelling the formation of today's massive ellipticals
- Globular Cluster Systems of Relic Galaxies
- Galaxy chemical evolution models: The role of molecular gas formation
- The fate of a red nugget: In-situ star formation of satellites around a massive compact galaxy
- The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
- Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies
- The evolution of cold neutral gas and the star formation history
- The supermassive black hole merger driven evolution of high-redshift red nuggets into present-day cored early-type galaxies
- Projected distances to host galaxy reduce SNIa dispersion
- The Puzzling Origin of Massive Compact Galaxies in MaNGA
- Bulgeless disks, dark galaxies, inverted color gradients, and other expected phenomena at higher z. The chromatic surface brightness modulation (CMOD) effect
- Spatially-resolved stellar populations and kinematics with KCWI: probing the assembly history of the massive early-type galaxy NGC 1407
- SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies
- Structural analysis of massive galaxies using HST deep imaging at z < 0.5
- The Size Evolution of Elliptical Galaxies
- Dynamical masses and non-homology of massive elliptical galaxies grown by dry mergers
- A possible connection between the spin temperature of damped Lyman-alpha absorption systems and star formation history
- The physical properties of massive green valley galaxies as a function of environments at in 3D-\textit{HST}/CANDELS fields
- The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies
- The merger history of massive spheroids since z~1 is size independent
- The central dark matter fraction of massive early-type galaxies
- The PSF Smoothing Effect on Concentration-Related Parameters of High Redshift Galaxies in HST and JWST
- The Fundamental Plane of Massive Quiescent Galaxies at z~2
- The galaxy ancestor problem
- Constraints on the evolutionary mechanisms of massive galaxies since from their velocity dispersions
- The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities
- HELLO project: High- Evolution of Large and Luminous Objects
- Probing the mass assembly of massive nearby galaxies with deep imaging
- A subarcsecond near-infrared view of massive galaxies at z > 1 with Gemini Multiconjugate Adaptive Optics
- Use of spatial cross correlation function to study formation mechanism of massive elliptical galaxies
- Extremely Low Molecular Gas Content in the Vicinity of a Red Nugget Galaxy at
- A spectroscopically confirmed z=1.327 galaxy-scale deflector magnifying a z~8 Lyman-Break galaxy in the Brightest of Reionizing Galaxies survey
- Total mass distributions of Sersic galaxies from photometry $&$ cent\ ral velocity dispersion
- Dark Matter Redistribution Explains Galaxy Growth and Rotation Curve Development
- Self-Similar Buildup and Inside-Out Growth: Tracing the Evolution of Intermediate to High-Mass Star-Forming Galaxies Since
- A Large Massive Quiescent Galaxy Sample at z~1.2
- A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn
- Exploring high-z galaxies with the E-ELT
- Compact dust-obscured star-formation and the origin of the galaxy bimodality
- Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn
- The size and mass evolution of the massive galaxies over cosmic time
- Dynamics of merging: Post-merger mixing and relaxation of an Illustris galaxy
- The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
- Capivara: A Spectral-based Segmentation Method for IFU Data Cubes
- The satellite population around luminous red galaxies in the 25 square degree DESI Legacy Imaging Surveys Early Data Release
- COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 m Since
- SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
- Velocity Dispersions and Stellar Populations of the Most Compact and Massive Early-Type Galaxies at Redshift ~1
- How do galaxies get their baryons?