YL
Yongming Liang
astro-ph.GAastro-ph.COastro-ph.IMastro-ph.SRcs.AI
On Valency
published · living versionsW_23mqsf45·v2 · currentpublished
Rest-frame Ultraviolet Variability of Quasars in the Cosmic Himalayas Overdensity
with Jiaqi Lin, Zhenya Zheng, Bin Ma, Lin Long
2 versions
Preprints & journals
27 papers in the corpus · 2018–2026Deeper detection limits in astronomical imaging using self-supervised spatiotemporal denoising.41712693 · Guo, Yuduo, Zhang, Hao, Li, Mingyu et al.2026 · 5 citationsScience (New York, N.Y.). 2026;392(6797):eady9404
Subaru High- Exploration of Low-Luminosity Quasars (SHELLQs). XXV. Large-scale environments of low-luminosity quasars at traced by Ly emitters2602.11736v2 · Junya Arita, Nobunari Kashikawa, Yoshiki Matsuoka et al.2026 · 0 citationsarXiv
Cosmic Himalayas in CROCODILE : Probing the Extreme Quasar Overdensities by Count-in-Cells analysis and Nearest Neighbor Distribution2512.24966v2 · Yuto Kuwayama, Yongming Liang, Kentaro Nagamine et al.2025 · 0 citationsarXiv
Little red dot variability over a century reveals black hole envelope via a giant Einstein cross2512.05180v1 · Zijian Zhang, Mingyu Li, Masamune Oguri et al.2025 · 2 citationsarXiv
JWST COSMOS-3D: Spectroscopic Census and Luminosity Function of [O III] Emitters at 6.75<z<9.05 in COSMOS2510.11373v3 · Romain A. Meyer, Feige Wang, Koki Kakiichi et al.2025 · 0 citationsarXiv
RIDEN pilot survey: broad-band selection of candidate quasars with extended Lyman- nebulae using CLAUDS-HSC-SSP-DUNES joint data2506.04570v1 · Rhythm Shimakawa, Satoshi Kikuta, Haruka Kusakabe et al.2025 · 0 citationsarXiv
Predicting Ly Emission from Distant Galaxies with Neural Network Architecture2412.14676v1 · Takehiro Yoshioka, Nobunari Kashikawa, Yoshihiro Takeda et al.2024 · 0 citationsarXiv
SILVERRUSH. XIV. Lya Luminosity Functions and Angular Correlation Functions from ~20,000 Lya Emitters at z~2.2-7.3 from upto 24 HSC-SSP and CHORUS Surveys: Linking the Post-Reionization Epoch to the Heart of Reionization2411.15495v1 · Hiroya Umeda, Masami Ouchi, Satoshi Kikuta et al.2024 · 0 citationsarXiv
Mining for Protoclusters at from Photometric Datasets with Deep Learning2411.11956v1 · Yoshihiro Takeda, Nobunari Kashikawa, Kei Ito et al.2024 · 0 citationsarXiv
The Physical Origin of Extreme Emission Line Galaxies at High redshifts: Strong {\sc [Oiii]} Emission Lines Produced by Obscured AGNs2410.12198v2 · Chenghao Zhu, Yuichi Harikane, Masami Ouchi et al.2024 · 0 citationsarXiv
Ly imaging around the hyperluminous dust-obscured quasar W2246$-$0526 at 2407.16971v1 · Yibin Luo, Lulu Fan, Yongming Liang et al.2024 · 3 citationsarXiv
MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Ly Nebulae at Cosmic Noon2405.13113v2 · Mingyu Li, Haibin Zhang, Zheng Cai et al.2024 · 10 citationsarXiv
Cosmic Himalayas: The Highest Quasar Density Peak Identified in a 10,000 deg Sky with Spatial Discrepancies between Galaxies, Quasars, and IGM HI2404.15963v2 · Yongming Liang, Masami Ouchi, Dongsheng Sun et al.2024 · 2 citationsarXiv
Subaru High- Exploration of Low-Luminosity Quasars (SHELLQs). XVIII. The Dark Matter Halo Mass of Quasars at 2307.02531v1 · Junya Arita, Nobunari Kashikawa, Yoshiki Matsuoka et al.2023 · 0 citationsarXiv
SILVERRUSH. XIII. A Catalog of 20,567 Ly Emitters at Identified in the Full-depth Data of the Subaru/HSC-SSP and CHORUS Surveys2305.08921v2 · Satoshi Kikuta, Masami Ouchi, Takatoshi Shibuya et al.2023 · 20 citationsarXiv
COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at 2301.08845v1 · Kei Ito, Masayuki Tanaka, Francesco Valentino et al.2023 · 51 citationsarXiv
MAMMOTH-Subaru III. Ly Halo Extended to kpc Identified by Stacking Ly Emitters at 2301.07358v1 · Haibin Zhang, Zheng Cai, Yongming Liang et al.2023 · 0 citationsarXiv
MAMMOTH-Subaru IV. Large Scale Structure and Clustering Analysis of Ly Emitters and Ly Blobs at 2301.07359v2 · Haibin Zhang, Zheng Cai, Mingyu Li et al.2023 · 7 citationsarXiv
MAMMOTH-Subaru V. Effects of Cosmic Variance on Ly Luminosity Functions at 2301.07360v1 · Ke Ma, Haibin Zhang, Zheng Cai et al.2023 · 6 citationsarXiv
The physical origin for spatially large scatter of IGM opacity at the end of reionization: the IGM Ly opacity-galaxy density relation2207.05098v1 · Rikako Ishimoto, Nobunari Kashikawa, Daichi Kashino et al.2022 · 18 citationsarXiv
CHORUS IV: Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC2201.07261v1 · Takehiro Yoshioka, Nobunari Kashikawa, Akio K. Inoue et al.2022 · 13 citationsarXiv
A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~42112.01684v1 · Hisakazu Uchiyama, Takuji Yamashita, Jun Toshikawa et al.2021 · 13 citationsarXiv
Third Data Release of the Hyper Suprime-Cam Subaru Strategic Program2108.13045v1 · Hiroaki Aihara, Yusra AlSayyad, Makoto Ando et al.2021 · 360 citationsarXiv
Interrelation of the environment of Ly emitters and massive galaxies at 2105.01670v1 · Kei Ito, Nobunari Kashikawa, Masayuki Tanaka et al.2021 · 15 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z~62009.06648v1 · Rikako Ishimoto, Nobunari Kashikawa, Masafusa Onoue et al.2020 · 23 citationsarXiv
Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program1905.12221v2 · Hiroaki Aihara, Yusra AlSayyad, Makoto Ando et al.2019 · 515 citationsarXiv
Suppression of Low-mass Galaxy Formation around Quasars at z~2-31811.03662v1 · H.Uchiyama, N.Kashikawa, R. Overzier et al.2018 · 16 citationsarXiv
Career total: at least 46 works. 27 are in this corpus.
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