GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with∼ 4,000,000 Galaxies at z∼ 2–7: Galaxy–AGN Transition, Star Formation Efficiency, and …

Y Harikane, Y Ono, M Ouchi, C Liu… - The Astrophysical …, 2022 - iopscience.iop.org
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 …

Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

IceCube Collaboration, MAGIC, AGILE, ASAS-SN… - Science, 2018 - science.org
INTRODUCTION Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and
traveling at nearly the speed of light, they can escape the densest environments and may be …

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 …

New constraints on Lyman-α opacity with a sample of 62 quasarsat z > 5.7

SEI Bosman, X Fan, L Jiang, S Reed… - Monthly Notices of …, 2018 - academic.oup.com
We present measurements of the mean and scatter of the intergalactic medium (IGM) Lyman-
α opacity at 4.9< z< 6.1 along the lines of sight of 62 quasars at z source> 5.7, the largest …

The Gemini–North Multi‐Object Spectrograph: Performance in imaging, long‐slit, and multi‐object spectroscopic modes

IM Hook, I Jørgensen, JR Allington‐Smith… - Publications of the …, 2004 - iopscience.iop.org
Results of the commissioning of the first Gemini Multi‐Object Spectrograph (GMOS) are
described. GMOS and the Gemini–North telescope act as a complete system to exploit a …

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 …

The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lyα emitters from z= 3.1 to 5.7 in the 1 deg2 field: luminosity functions and AGN

M Ouchi, K Shimasaku, M Akiyama… - The Astrophysical …, 2008 - iopscience.iop.org
We present luminosity functions (LFs) and various properties of Lyα emitters (LAEs) at z=
3.1, 3.7, and 5.7, in a 1 deg 2 sky of the Subaru/XMM–Newton Deep Survey (SXDS) Field …

Subaru high-z exploration of low-luminosity quasars (SHELLQs). XVIII. The dark matter halo mass of quasars at z∼ 6

J Arita, N Kashikawa, Y Matsuoka, W He… - The Astrophysical …, 2023 - iopscience.iop.org
We present, for the first time, dark matter halo (DMH) mass measurement of quasars at z∼ 6
based on a clustering analysis of 107 quasars. Spectroscopically identified quasars are …

Completing the census of Lyα emitters at the reionization epoch

N Kashikawa, K Shimasaku, Y Matsuda… - The Astrophysical …, 2011 - iopscience.iop.org
We carried out extended spectroscopic confirmations of Lyα emitters (LAEs) at z= 6.5 and
5.7 in the Subaru Deep Field. Now, the total number of spectroscopically confirmed LAEs is …

The end of the reionization epoch probed by Lyα emitters at z= 6.5 in the Subaru Deep Field

N Kashikawa, K Shimasaku, MA Malkan… - The Astrophysical …, 2006 - iopscience.iop.org
We report an extensive search for Lyα emitters (LAEs) at z= 6.5 in the Subaru Deep Field.
Subsequent spectroscopy with Subaru and Keck identified eight more LAEs, giving a total of …