MOIRCS Deep Survey. VII. NIR morphologies of star-forming galaxies at redshift z ∼ 1.

@article{Konishi2010MOIRCSDS,
  title={MOIRCS Deep Survey. VII. NIR morphologies of star-forming galaxies at redshift z ∼ 1.},
  author={Masahiro Konishi and Masayuki Akiyama and Masaru Kajisawa and Takashi Ichikawa and Ryuji Suzuki and Chihiro Tokoku and Yuka Katsuno Uchimoto and Tomohiro Yoshikawa and Ichi Tanaka and Masato Onodera and Masami Ouchi and Koji Omata and Tetsuo Nishimura and Toru Yamada},
  journal={Publications of the Astronomical Society of Japan},
  year={2010},
  volume={63}
}
We investigated rest-frame near-infrared (NIR) morphologies of a sample of 139 galaxies with Ms � 1 � 10 10 Mˇ at z = 0.8-1.2 in the GOODS-North field using our deep NIR imaging data (MOIRCS Deep Survey, MODS). We focused on Luminous Infrared Galaxies (LIRGs), which dominate a high star formation rate (SFR) density at z � 1, in a sample identified by cross-correlating with the Spitzer/MIPS 24 � m source catalog. We performed two- dimensional light profile fittings of z � 1 galaxies in the Ks… Expand
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References

SHOWING 1-10 OF 64 REFERENCES
MOIRCS DEEP SURVEY. IV. EVOLUTION OF GALAXY STELLAR MASS FUNCTION BACK TO z ∼ 3
We use very deep near-infrared (NIR) imaging data obtained in MOIRCS Deep Survey (MODS) to investigate the evolution of the galaxy stellar mass function back to z ~ 3. The MODS data reach J = 24.2, HExpand
Toward an Understanding of the Rapid Decline of the Cosmic Star Formation Rate
We present a first analysis of deep 24 μm observations with the Spitzer Space Telescope of a sample of nearly 1500 galaxies in a thin redshift slice, 0.65 ≤ z < 0.75. We combine the infrared dataExpand
TRIGGERED OR SELF-REGULATED STAR FORMATION WITHIN INTERMEDIATE REDSHIFT LUMINOUS INFRARED GALAXIES. I. MORPHOLOGIES AND SPECTRAL ENERGY DISTRIBUTIONS
As part of the Center for Adaptive Optics (AO) Treasury Survey (CATS) we imaged a set of 15 intermediate redshift (z ~ 0.8) luminous infrared (IR) galaxies (LIRGs) with the Keck Laser Guide StarExpand
Luminous Infrared Galaxies in the Local Universe
We study the morphology and star formation properties of 159 local luminous infrared galaxies (LIRGs) using multicolor images from Data Release 2 (DR2) of the Sloan Digital Sky Survey (SDSS). TheExpand
GEMS: The Surface Brightness and Surface Mass Density Evolution of Disk Galaxies
We combine HST imaging from the GEMS (Galaxy Evolution from Morphologies and SEDs) survey with photometric redshifts from COMBO-17 to explore the evolution of disk-dominated galaxies since z 1.1. TheExpand
Optical Morphology Evolution of Infrared Luminous Galaxies in GOODS-N
We combine optical morphologies and photometry from HST, redshifts from Keck, and mid-infrared luminosities from Spitzer for an optically selected sample of ~800 galaxies in GOODS-N to track theExpand
The 0.4 < z < 1.3 star formation history of the Universe as viewed in the far-infrared
Aims. We use the deepest existing mid- and far-infrared observations (reaching ∼3 mJy at 70 μm) obtained with Spitzer in the Great Observatories Origins Deep Survey (GOODS) and Far Infrared DeepExpand
Exploring the Evolutionary Paths of the Most Massive Galaxies since z ~ 2
We use Spitzer MIPS data from the FIDEL Legacy Project in the extended Groth strip to analyze the stellar mass assembly of massive ( -->M > 1011 M☉) galaxies at -->z z = 1–2 are detected at 24 μm,Expand
Infrared Spectral Energy Distributions of z ~ 0.7 Star-forming Galaxies
We analyze the infrared (IR) spectral energy distributions (SEDs) for 10 μm < λrest < 100 μm for ~600 galaxies at z ~ 0.7 in the extended Chandra Deep Field South by stacking their Spitzer 24, 70,Expand
Infrared Luminosity Functions from the Chandra Deep Field-South: The Spitzer View on the History of Dusty Star Formation at 0 ≲ z ≲ 1*
We analyze a sample of ~2600 Spitzer MIPS 24 μm sources brighter than ~80 μJy and located in the Chandra Deep Field-South to characterize the evolution of the comoving infrared (IR) energy density ofExpand
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