NK
N. Kashikawa
astro-ph.GAastro-phastro-ph.COastro-ph.HEastro-ph.IMastro-ph.EPastro-ph.SR
On Valency
published · living versionsW_e6dcd5te·v1 · currentpublished
The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
with N. Suzuki, D. Rubin, C. Lidman, G. Aldering +60
1 version
Preprints & journals
197 papers in the corpus · 1998–2026Probing Spatial Variations in IGM Transmission: Higher Ly Visibility in an H-Selected Galaxy Overdensity at 2609.35221v1 · Shunta Shimizu, Nobunari Kashikawa, Junya Arita et al.2026 · 0 citationsarXiv
SHELLQs. Black Hole Mass and Eddington Ratio Distributions of Intermediate-Luminosity Quasars at 6<z<72609.09266v1 · Masafusa Onoue, John D. Silverman, Yoshiki Matsuoka et al.2026 · 0 citationsarXiv
H I Absorbers as Beacons of Hidden Structure at : Multi-Component, Metal-Rich Absorption System near a Protocluster2609.04349v1 · Kentaro Koretomo, Nobunari Kashikawa, Toru Misawa et al.2026 · 0 citationsarXiv
Subaru meets JWST: A Direct Measurement of Ly Escape Fraction at with Dual Narrow-Band Imaging2607.08264v1 · Shunta Shimizu, Nobunari Kashikawa, Ryo Emori et al.2026 · 0 citationsarXiv
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
SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z > 6 Quasar Host Galaxies using the JWST NIRSpec Fixed Slit2510.22403v1 · Camryn L. Phillips, Michael A. Strauss, Masafusa Onoue et al.2025 · 4 citationsarXiv
HST Confirms Sub-5 kpc Dual Quasar Pairs at Cosmic Noon2510.09059v2 · Qian Wang, Xuheng Ding, John Silverman et al.2025 · 3 citationsarXiv
Serendipitous Discovery of an Optically-Dark Ultra-Luminous Infrared Galaxy at = 3.42510.00590v1 · N. H. Hayatsu, Zhi-Yu Zhang, R. J. Ivison et al.2025 · 0 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at 2508.21229v2 · Yoshiki Matsuoka, Kazushi Iwasawa, Masafusa Onoue et al.2025 · 0 citationsApJS 280, 68 (2025)
SHELLQs-JWST perspective on the intrinsic mass relation between supermassive black holes and their host galaxies at z > 62507.23066v2 · John Silverman, Junyao Li, Xuheng Ding et al.2025 · 15 citationsarXiv
Age dependence of Ly\alpha\ escape fraction of Ly\alpha\ emitters and their significant role in cosmic reionization2506.03242v2 · Shunta Shimizu, Nobunari Kashikawa, Satoshi Kikuta et al.2025 · 6 citationsMon Not R Astron Soc (2025) 3125-3143
SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 62505.04825v3 · Yoshiki Matsuoka, Masafusa Onoue, Kazushi Iwasawa et al.2025 · 13 citationsApJ 988, 57 (2025)
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) XXII. Chandra observations of narrow-line quasar candidates at z>62505.04826v3 · K. Iwasawa, R. Gilli, F. Vito et al.2025 · 1 citationarXiv
SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>62505.03876v2 · Xuheng Ding, Masafusa Onoue, John D. Silverman et al.2025 · 11 citations2025ApJ, 993, 91D
Subaru High- Exploration of Low-Luminosity Quasars (SHELLQs). XXIII. The powering mechanisms of the Ly haloes around high- quasars probed by slit spectroscopy2504.05984v1 · Hiroki Hoshi, Rikako Ishimoto, Nobunari Kashikawa 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
Mining for Protoclusters at from Photometric Datasets with Deep Learning2411.11956v1 · Yoshihiro Takeda, Nobunari Kashikawa, Kei Ito et al.2024 · 0 citationsarXiv
The nature of low-luminosity AGNs discovered by JWST based on clustering analysis: progenitors of low- quasars?2410.08707v2 · Junya Arita, Nobunari Kashikawa, Masafusa Onoue et al.2024 · 20 citationsarXiv
A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z>62409.07113v2 · Masafusa Onoue, Xuheng Ding, John D. Silverman et al.2024 · 25 citationsarXiv
JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe2406.18352v2 · Yuichi Harikane, Akio K. Inoue, Richard S. Ellis et al.2024 · 102 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
Discovery of merging twin quasars at z = 6.052405.02465v1 · Yoshiki Matsuoka, Takuma Izumi, Masafusa Onoue et al.2024 · 19 citationsThe Astrophysical Journal Letters, Volume 965, Issue 1, id.L4, 8 pp (2024)
Galaxy properties from the outskirts to the core of a protocluster at z=3.6992404.15910v1 · Jun Toshikawa, Stijn Wuyts, Nobunari Kashikawa et al.2024 · 0 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
Black hole mass and Eddington ratio distributions of less-luminous quasars at in the Subaru Hyper Suprime-Cam Wide field2311.08922v1 · Wanqiu He, Masayuki Akiyama, Motohiro Enoki et al.2023 · 1 citationarXiv
Subaru High- Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at Estimated via Spectral Comparison with Low- Quasars2310.12222v1 · Ayumi Takahashi, Yoshiki Matsuoka, Masafusa Onoue et al.2023 · 0 citationsarXiv
An enhanced abundance of bright galaxies in protocluster candidates at z~3-52310.08525v1 · Jun Toshikawa, Stijn Wuyts, Nobunari Kashikawa et al.2023 · 18 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
Quasar Luminosity Function at z = 72305.11225v1 · Yoshiki Matsuoka, Masafusa Onoue, Kazushi Iwasawa et al.2023 · 66 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
Updated measurements of [O III] 88 m, [C II] 158 m, and Dust Continuum Emission from a z=7.2 Galaxy2302.02365v2 · Yi W. Ren, Yoshinobu Fudamoto, Akio K. Inoue et al.2023 · 12 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
X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z=6.562211.13820v1 · Julien Wolf, Kirpal Nandra, Mara Salvato et al.2022 · 18 citationsA&A 669, A127 (2023)
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
Exploratory Study of Transverse Proximity Effect around BAL Quasars2206.10871v1 · Toru Misawa, Rikako Ishimoto, Satoshi Kobu et al.2022 · 2 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
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.02111.12766v1 · Yoshiki Matsuoka, Kazushi Iwasawa, Masafusa Onoue et al.2021 · 61 citationsarXiv
The SSA22 HI Tomography Survey (SSA22-HIT). I. Data Set and Compiled Redshift Catalog2110.11977v3 · Ken Mawatari, Akio K. Inoue, Toru Yamada et al.2021 · 4 citationsarXiv
Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data2110.05011v2 · Takumi S. Tanaka, Rhythm Shimakawa, Kazuhiro Shimasaku et al.2021 · 9 citationsPASJ 74 (2022) 1-23
Ionizing radiation from AGNs at z>3.3 with the Subaru Hyper Suprime-Cam Survey and the CFHT Large Area U-band Deep Survey (CLAUDS)2109.10138v1 · Ikuru Iwata, Marcin Sawicki, Akio K. Inoue et al.2021 · 14 citationsarXiv
SILVERRUSH. XI. Intensity Mapping for Lya Emission Extending over comoving kpc around LAEs with Subaru HSC-SSP and CHORUS Data2108.09288v1 · Shotaro Kikuchihara, Yuichi Harikane, Masami Ouchi et al.2021 · 16 citationsarXiv
GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ~4,000,000 Galaxies at z~2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z>102108.01090v3 · Yuichi Harikane, Yoshiaki Ono, Masami Ouchi et al.2021 · 202 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIV. A Candidate Type-II Quasar at z=6.12922106.13807v1 · Masafusa Onoue, Yoshiki Matsuoka, Nobunari Kashikawa et al.2021 · 20 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
Catch Me if You Can: Biased Distribution of Ly-emitting Galaxies according to the Viewing Direction2104.10580v1 · Rieko Momose, Kazuhiro Shimasaku, Kentaro Nagamine et al.2021 · 16 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIII. Large-scale Feedback and Star Formation in a Low-Luminosity Quasar at z = 7.07 on the Local Black Hole to Host Mass Relation2104.05738v2 · Takuma Izumi, Yoshiki Matsuoka, Seiji Fujimoto et al.2021 · 85 citationsarXiv
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