Yongming Liang
03 / PUBLICATIONS

Papers & preprints

34 refereed articles · 4 preprints

2026

  1. Preprint

    Subaru meets JWST: A Direct Measurement of Lyα Escape Fraction at z ≃ 6.2 with Dual Narrow-Band Imaging

    Shimizu, Shunta et al.

    arXiv:2607.08264

    ADSDOIarXiv

  2. JWST COSMOS-3D: Spectroscopic census and luminosity function of [O III] emitters at 6.75 < z < 9.05 in COSMOS

    Meyer, Romain A. et al.

    A&A, 712, A16

    ADSDOIarXiv
  3. Preprint

    Prime Focus Spectrograph on the Subaru Telescope: Overview of Science Operations

    Tanaka, Masayuki et al.

    arXiv:2606.14012

    ADSDOIarXiv

  4. Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) — XXV. Large-scale environments of low-luminosity quasars at z ∼ 6 traced by Lyα emitters

    Arita, Junya et al.

    MNRAS, 549, stag784

    ADSDOIarXiv

  5. Cosmic Himalayas in CROCODILE: Probing the Extreme Quasar Overdensities by Count-in-cells Analysis and Nearest-neighbor Distribution

    Kuwayama, Yuto et al.

    ApJ, 1001, 172

    ADSDOIarXiv
  6. Preprint

    A Python-Based Peeling Framework for Radio Interferometry: Application to uGMRT 650MHz Imaging

    Peng, Hao et al.

    arXiv:2603.10758

    ADSDOIarXiv

  7. Deeper detection limits in astronomical imaging using self-supervised spatiotemporal denoising

    Guo, Yuduo et al.

    Science, 392, eady9404

    ADSDOIarXiv

2025

  1. Preprint

    Little red dot variability over a century reveals black hole envelope via a giant Einstein cross

    Zhang, Zijian et al.

    arXiv:2512.05180

    ADSDOIarXiv

  2. RIDEN pilot survey: broad-band selection of candidate quasars with extended Lyman-α nebulae using CLAUDS–HSC-SSP–DUNES² joint data

    Shimakawa, Rhythm et al.

    MNRAS, 540, 3565–3582

    ADSDOIarXiv

  3. Cosmic Himalayas: The Highest Quasar Density Peak Identified in a 10,000 deg² Sky with Spatial Discrepancies between Galaxies, Quasars, and IGM H I

    Liang, Yongming et al.

    ApJ, 986, 60

    ADSDOIarXiv

  4. SILVERRUSH. XIV. Lyα Luminosity Functions and Angular Correlation Functions from ∼20,000 Lyα Emitters at z ∼ 2.2–7.3 from up to 24 deg² HSC-SSP and CHORUS Surveys: Linking the Postreionization Epoch to the Heart of Reionization

    Umeda, Hiroya et al.

    ApJS, 277, 37

    ADSDOIarXiv

  5. The Physical Origin of Extreme Emission Line Galaxies at High Redshifts: Strong [O III] Emission Lines Produced by Obscured Active Galactic Nuclei

    Zhu, Chenghao et al.

    ApJ, 982, 27

    ADSDOIarXiv

  6. MAMMOTH-Subaru. IV. Large Scale Structure and Clustering Analysis of Lyα Emitters and Lyα Blobs at z = 2.2–2.3

    Zhang, Haibin et al.

    ApJ, 981, 70

    ADSDOIarXiv

  7. Predicting Lyα emission from distant galaxies with neural network architecture

    Yoshioka, Takehiro et al.

    MNRAS, 536, 3386–3400

    ADSDOIarXiv

2024

  1. MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Lyα Nebulae at Cosmic Noon

    Li, Mingyu et al.

    ApJS, 275, 27

    ADSDOIarXiv

  2. Mining for Protoclusters at z ∼ 4 from Photometric Data Sets with Deep Learning

    Takeda, Yoshihiro et al.

    ApJ, 977, 81

    ADSDOIarXiv

  3. Lyα Imaging around the Hyperluminous Dust-obscured Quasar W2246–0526 at z = 4.6

    Luo, Yibin et al.

    ApJ, 972, 51

    ADSDOIarXiv

  4. MAMMOTH-Subaru. V. Effects of Cosmic Variance on Lyα Luminosity Functions at z = 2.2–2.3

    Ma, Ke et al.

    ApJ, 961, 102

    ADSDOIarXiv

  5. MAMMOTH-Subaru. III. Lyα Halo Identified by Stacking ∼3300 Lyα Emitters at z = 2.2–2.3

    Zhang, Haibin et al.

    ApJ, 961, 63

    ADSDOIarXiv

2023

  1. SILVERRUSH. XIII. A Catalog of 20,567 Lyα Emitters at z = 2–7 Identified in the Full-depth Data of the Subaru/HSC-SSP and CHORUS Surveys

    Kikuta, Satoshi et al.

    ApJS, 268, 24

    ADSDOIarXiv

  2. Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVIII. The Dark Matter Halo Mass of Quasars at z ∼ 6

    Arita, Junya et al.

    ApJ, 954, 210

    ADSDOIarXiv

  3. COSMOS2020: Discovery of a Protocluster of Massive Quiescent Galaxies at z = 2.77

    Ito, Kei et al.

    ApJL, 945, L9

    ADSDOIarXiv

2022

  1. The physical origin for spatially large scatter of IGM opacity at the end of reionization: The IGM Lyα opacity-galaxy density relation

    Ishimoto, Rikako et al.

    MNRAS, 515, 5914–5926

    ADSDOIarXiv

  2. Third data release of the Hyper Suprime-Cam Subaru Strategic Program

    Aihara, Hiroaki et al.

    PASJ, 74, 247–272

    ADSDOIarXiv

  3. CHORUS. IV. Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC

    Yoshioka, Takehiro et al.

    ApJ, 927, 32

    ADSDOIarXiv

  4. A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed Out by High-z Radio Galaxies at z ∼ 4

    Uchiyama, Hisakazu et al.

    ApJ, 926, 76

    ADSDOIarXiv

2021

  1. Interrelation of the Environment of Lyα Emitters and Massive Galaxies at 2 < z < 4.5

    Ito, Kei et al.

    ApJ, 916, 35

    ADSDOIarXiv

  2. Probing Feedback via IGM tomography and the Lyα Forest with Subaru PFS, TMT/ELT, and JWST

    Nagamine, Kentaro et al.

    ApJ, 914, 66

    ADSDOIarXiv

  3. SILVERRUSH X: Machine Learning-aided Selection of 9318 LAEs at z = 2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 from the HSC SSP and CHORUS Survey Data

    Ono, Yoshiaki et al.

    ApJ, 911, 78

    ADSDOIarXiv

  4. Evidence for GN-z11 as a luminous galaxy at redshift 10.957

    Jiang, Linhua et al.

    Nature Astronomy, 5, 256–261

    ADSDOIarXiv

  5. Statistical Correlation between the Distribution of Lyα Emitters and Intergalactic Medium H I at z ∼ 2.2 Mapped by the Subaru/Hyper Suprime-Cam

    Liang, Yongming et al.

    ApJ, 907, 3

    ADSDOIarXiv

2020

  1. CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview

    Inoue, Akio K. et al.

    PASJ, 72, 101

    ADSDOIarXiv

  2. Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ∼ 4

    Uchiyama, Hisakazu et al.

    ApJ, 905, 125

    ADSDOIarXiv

  3. Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z ∼ 6

    Ishimoto, Rikako et al.

    ApJ, 903, 60

    ADSDOIarXiv

  4. The UV Luminosity Function of Protocluster Galaxies at z ∼ 4: The Bright-end Excess and the Enhanced Star Formation Rate Density

    Ito, Kei et al.

    ApJ, 899, 5

    ADSDOIarXiv

2019

  1. Second data release of the Hyper Suprime-Cam Subaru Strategic Program

    Aihara, Hiroaki et al.

    PASJ, 71, 114

    ADSDOIarXiv

  2. The Brightest UV-selected Galaxies in Protoclusters at z ∼ 4: Ancestors of Brightest Cluster Galaxies?

    Ito, Kei et al.

    ApJ, 878, 68

    ADSDOIarXiv

  3. Suppression of Low-mass Galaxy Formation around Quasars at z ∼ 2–3

    Uchiyama, Hisakazu et al.

    ApJ, 870, 45

    ADSDOIarXiv

8 years · 38 papers & preprints