Masami Ouchi
0000-0002-1049-6658
University of Tokyo
203 papers found
Refreshing results…
ALMA Reveals Strong $[{\bf{C}}\,{\bf{II}}]$ Emission in a Galaxy Embedded in a Giant LyαBlob atz= 3.1
Imaging of diffuse H i absorption structure in the SSA22 proto-cluster region at $z$ = 3.1
A new quadruple gravitational lens from the Hyper Suprime-Cam Survey: the puzzle of HSC J115252+004733
A HARD IONIZING SPECTRUM IN Z = 3–4 Ly α EMITTERS WITH INTENSE $[{\Rm{O}}\,{\rm{III}}]$ EMISSION: ANALOGS OF GALAXIES IN THE REIONIZATION ERA?
SUBARU HIGH-zEXPLORATION OF LOW-LUMINOSITY QUASARS (SHELLQs). I. DISCOVERY OF 15 QUASARS AND BRIGHT GALAXIES AT 5.7
BRIGHT AND FAINT ENDS OF LyαLUMINOSITY FUNCTIONS ATz= 2 DETERMINED BY THE SUBARU SURVEY: IMPLICATIONS FOR AGNs, MAGNIFICATION BIAS, AND ISM H I EVOLUTION
A NEW CONSTRAINT ON THE LyαFRACTION OF UV VERY BRIGHT GALAXIES AT REDSHIFT 7
A VERY COMPACT DENSE GALAXY OVERDENSITY WITHδ≃ 130 IDENTIFIED ATz∼ 8: IMPLICATIONS FOR EARLY PROTOCLUSTER AND CLUSTER CORE FORMATION
EVOLUTION OF STELLAR-TO-HALO MASS RATIO ATz= 0–7 IDENTIFIED BY CLUSTERING ANALYSIS WITH THE HUBBLE LEGACY IMAGING AND EARLY SUBARU/HYPER SUPRIME-CAM SURVEY DATA
MORPHOLOGIES OF ∼190,000 GALAXIES ATz= 0–10 REVEALED WITHHSTLEGACY DATA. II. EVOLUTION OF CLUMPY GALAXIES
Precise Strong Lensing Mass Modeling of Fourhubblefrontier Field Clusters and a Sample of Magnified High-Redshift Galaxies
Large scale profiles of galaxies at z=0-2 studied by stacking the HSC SSP survey data
Statistical properties of diffuse Lyα haloes around star-forming galaxies atz∼ 2
ALMA CENSUS OF FAINT 1.2 Mm SOURCES DOWN TO ∼ 0.02 mJy: EXTRAGALACTIC BACKGROUND LIGHT AND DUST-POOR, HIGH-zGALAXIES
PHYSICAL PROPERTIES OF SPECTROSCOPICALLY CONFIRMED GALAXIES ATz≥ 6. III. STELLAR POPULATIONS FROM SED MODELING WITH SECURE LyαEMISSION AND REDSHIFTS
A CLOSE COMPARISON BETWEEN OBSERVED AND MODELED LyαLINES FORz∼ 2.2 LyαEMITTERS
Evolution of star formation in the UKIDSS Ultra Deep Survey Field – II. Star formation as a function of stellar mass betweenz = 1.46 and 0.63
MORPHOLOGIES OF ∼190,000 GALAXIES AT Z = 0–10 REVEALED WITH HST LEGACY DATA. I. SIZE EVOLUTION
The Subaru–XMM-Newton Deep Survey (SXDS). VIII. Multi-wavelength identification, optical/NIR spectroscopic properties, and photometric redshifts of X-ray sources
Deep rest-frame far-UV spectroscopy of the giant Lyman α emitter ‘Himiko’
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