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 …
Statistics of 207 Lyα emitters at a redshift near 7: constraints on reionization and galaxy formation models
M Ouchi, K Shimasaku, H Furusawa… - The Astrophysical …, 2010 - iopscience.iop.org
We present the Lyα luminosity function (LF), clustering measurements, and Lyα line profiles
based on the largest sample to date of 207 Lyα emitters (LAEs) at z= 6.6 on the 1 deg 2 sky …
based on the largest sample to date of 207 Lyα emitters (LAEs) at z= 6.6 on the 1 deg 2 sky …
The dark side of the halo occupation distribution
We analyze the halo occupation distribution (HOD) and two-point correlation function of
galaxy-size dark matter halos using high-resolution dissipationless simulations of the …
galaxy-size dark matter halos using high-resolution dissipationless simulations of the …
Identification of the brightest Lyα emitters at z= 6.6: implications for the evolution of the luminosity function in the reionization era
Using wide-field narrow-band surveys, we provide a new measurement of the z= 6.6
Lymanα emitter (LAE) luminosity function (LF), which constraints the bright end for the first …
Lymanα emitter (LAE) luminosity function (LF), which constraints the bright end for the first …
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 …
The LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxies
We present a measurement of the spatial clustering of submillimetre galaxies (SMGs) at z= 1–
3. Using data from the 870 μm Large APEX Bolometer Camera (LABOCA) submillimetre …
3. Using data from the 870 μm Large APEX Bolometer Camera (LABOCA) submillimetre …
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
We present clustering analysis results from 10,381 Lyman break galaxies (LBGs) at z∼ 4–7,
identified in the Hubble legacy deep imaging and new complimentary large-area …
identified in the Hubble legacy deep imaging and new complimentary large-area …
Cosmic evolution of quasar clustering: implications for the host haloes
C Porciani, M Magliocchetti… - Monthly Notices of the …, 2004 - academic.oup.com
We present detailed clustering measurements from the 2dF Quasi-Stellar Object Redshift
Survey (2QZ) in the redshift range 0.8< z< 2.1. Using a flux-limited sample of∼ 14 000 …
Survey (2QZ) in the redshift range 0.8< z< 2.1. Using a flux-limited sample of∼ 14 000 …
Subaru Deep Survey. VI. A Census of Lyman Break Galaxies at z≃ 4 and 5 in the Subaru Deep Fields: Clustering Properties
M Ouchi, K Shimasaku, S Okamura… - The Astrophysical …, 2004 - iopscience.iop.org
We investigate the clustering properties of 2600 Lyman break galaxies (LBGs) at z= 3.5-5.2
in two large blank fields, the Subaru Deep Field and the Subaru/XMM-Newton Deep Field …
in two large blank fields, the Subaru Deep Field and the Subaru/XMM-Newton Deep Field …
The Large-Scale and Small-Scale Clustering of Lyman Break Galaxies at 3.5⩽ z⩽ 5.5 from the GOODS Survey
We report on the angular correlation function of Lyman break galaxies (LBGs) at z~ 4 and 5
from deep samples obtained from the Great Observatories Deep Origins Survey (GOODS) …
from deep samples obtained from the Great Observatories Deep Origins Survey (GOODS) …