GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with∼ 4,000,000 Galaxies at z∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and …
We present new measurements of rest-UV luminosity functions and angular correlation
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …
Large Population of ALMA Galaxies at z> 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?
Y Harikane, M Ouchi, AK Inoue… - The Astrophysical …, 2020 - iopscience.iop.org
We present our new Atacama Large Millimeter/Submillimeter Array (ALMA) observations
targeting [O iii] 88 μm,[C ii] 158 μm,[N ii] 122 μm, and dust-continuum emission for three …
targeting [O iii] 88 μm,[C ii] 158 μm,[N ii] 122 μm, and dust-continuum emission for three …
Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z∼ 4–7 derived with the half-million dropouts on the 100 …
Y Ono, M Ouchi, Y Harikane… - Publications of the …, 2018 - academic.oup.com
We study the UV luminosity functions (LFs) at z∼ 4, 5, 6, and 7 based on the deep large-
area optical images taken by the Hyper Suprime-Cam (HSC) Subaru Strategic Program …
area optical images taken by the Hyper Suprime-Cam (HSC) Subaru Strategic Program …
Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program strategy and clustering properties …
M Ouchi, Y Harikane, T Shibuya… - Publications of the …, 2018 - academic.oup.com
We present the SILVERRUSH program strategy and clustering properties investigated
with∼ 2000 Lyα emitters (LAEs) at z= 5.7 and 6.6 found in the early data of the Hyper …
with∼ 2000 Lyα emitters (LAEs) at z= 5.7 and 6.6 found in the early data of the Hyper …
SILVERRUSH. IV. Lyα luminosity functions at z = 5.7 and 6.6 studied with ∼1300 Lyα emitters on the 14–21 deg2 sky
A Konno, M Ouchi, T Shibuya, Y Ono… - Publications of the …, 2018 - academic.oup.com
We present the Lyα luminosity functions (LFs) at z= 5.7 and 6.6 derived from a new large
sample of 1266 Lyα emitters (LAEs) identified in total areas of 14 and 21 deg2, respectively …
sample of 1266 Lyα emitters (LAEs) identified in total areas of 14 and 21 deg2, respectively …
Spectroscopic Confirmation of a Protocluster at z= 3.37 with a High Fraction of Quiescent Galaxies
Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …
SILVERRUSH. V. Census of Lyα,[O iii] λ5007, Hα, and [C ii] 158 μm Line Emission with∼ 1000 LAEs at z= 4.9–7.0 Revealed with Subaru/HSC
Y Harikane, M Ouchi, T Shibuya, T Kojima… - The Astrophysical …, 2018 - iopscience.iop.org
We investigate Lyα,[O iii] λ5007, Hα, and [C ii] 158 μm emission from 1124 galaxies at z= 4.9–
7.0. Our sample is composed of 1092 Lyα emitters (LAEs) at z= 4.9, 5.7, 6.6, and 7.0 …
7.0. Our sample is composed of 1092 Lyα emitters (LAEs) at z= 4.9, 5.7, 6.6, and 7.0 …
A lensed protocluster candidate at z= 7.66 identified in JWST observations of the galaxy cluster SMACS0723− 7327
Context. According to the current paradigm of galaxy formation, the first galaxies likely
formed within large dark matter haloes. The fragmentation of these massive haloes led to the …
formed within large dark matter haloes. The fragmentation of these massive haloes led to the …
GOLDRUSH. II. Clustering of galaxies at z ∼ 4–6 revealed with the half-million dropouts over the 100 deg2 area corresponding to 1 Gpc3
We present clustering properties from 579492 Lyman-break galaxies (LBGs) at z∼ 4–6 over
the 100 deg2 sky (corresponding to a 1.4 Gpc3 volume) identified in early data of the Hyper …
the 100 deg2 sky (corresponding to a 1.4 Gpc3 volume) identified in early data of the Hyper …
A Protocluster of Massive Quiescent Galaxies at z= 4
M Tanaka, M Onodera, R Shimakawa… - The Astrophysical …, 2024 - iopscience.iop.org
We report on discovery of a concentration of massive quiescent galaxies located at z= 4. The
concentration is first identified using high-quality photometric redshifts based on deep …
concentration is first identified using high-quality photometric redshifts based on deep …