:: Library Catalog

Cover Image

Saved in:

Bibliographic Details
Main Authors:	Toshikawa, Jun, Wuyts, Stijn, Kashikawa, Nobunari, Uchiyama, Hisakazu, Bremer, Malcolm, Sawicki, Marcin, Ono, Yoshiaki, Kubo, Mariko, Ito, Kei
Format:	Preprint
Published:	2024
Subjects:	Astrophysics of Galaxies
Online Access:	https://arxiv.org/abs/2404.15910
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

Mining for Protoclusters at $z\sim4$ from Photometric Datasets with Deep Learning
by: Takeda, Yoshihiro, et al.
Published: (2024)

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). X. The Massive and Passive Nature of Radio Galaxies at $z \sim 4$
by: Yamamoto, Yuta, et al.
Published: (2024)

Environments around quasars at $z\sim$3 revealed by wide-field imaging with Subaru HSC and CFHT
by: Suzuki, Yuta, et al.
Published: (2024)

Environment of SDSS quasars at $z=0.4$$-$$1.0$ explored by Subaru HSC
by: Shibata, Kohei, et al.
Published: (2025)

Predicting Ly$α$ Emission from Distant Galaxies with Neural Network Architecture
by: Yoshioka, Takehiro, et al.
Published: (2024)

The nature of low-luminosity AGNs discovered by JWST based on clustering analysis: progenitors of low-$z$ quasars?
by: Arita, Junya, et al.
Published: (2024)

Probing the stellar populations and star formation history of early-type galaxies at $0 < z < 1.1$ in the rest-frame ultraviolet
by: Ali, Sadman, et al.
Published: (2024)

Quasar Negative Feedback to Surrounding Galaxies Probed with Ly$α$ Emitters and Continuum-Selected Galaxies
by: Suzuki, Yuta, et al.
Published: (2025)

ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09
by: Huang, Shuo, et al.
Published: (2025)

The Galaxy Stellar Mass-SFR-Size Relation in EAGLE, TNG100, and Observations
by: Chu, Jiani, et al.
Published: (2026)

Serendipitous Discovery of an Optically-Dark Ultra-Luminous Infrared Galaxy at $z$ = 3.4
by: Hayatsu, N. H., et al.
Published: (2025)

Active Galactic Nuclei in a Mid-Infrared Selected Galaxy Sample at z>0.13: [Ne V]3426 Line Emission as a Benchmark
by: Li, Zi-Jian, et al.
Published: (2024)

Narrowband Imaging of a z=3.24 Protocluster: Insights from [O III] Emitting Galaxies
by: Shi, Ke, et al.
Published: (2025)

A Close Look at Ly$α$ Emitters with JWST/NIRCam at $z\approx3.1$
by: Liu, Yixiao, et al.
Published: (2023)

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 Universe
by: Harikane, Yuichi, et al.
Published: (2024)

The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
by: He, Kaimin, et al.
Published: (2026)

Age dependence of Lyα escape fraction of Lyα emitters and their significant role in cosmic reionization
by: Shimizu, Shunta, et al.
Published: (2025)

ADF22-WEB: Detection of a molecular gas reservoir in a massive quiescent galaxy located in a $z\approx3$ proto-cluster core
by: Umehata, Hideki, et al.
Published: (2025)

SE3D: Testing the recovery of stellar population, dust and structural properties on mock-observed toy model and simulated galaxies
by: Zhang, Junkai, et al.
Published: (2025)

The role of small-scale environments in the quenching of massive galaxies at $1<z<5$
by: Kakimoto, Takumi, et al.
Published: (2026)

Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs). XXV. Large-scale environments of low-luminosity quasars at $z\sim6$ traced by Ly$α$ emitters
by: Arita, Junya, et al.
Published: (2026)

SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6
by: Matsuoka, Yoshiki, et al.
Published: (2025)

Census for the Rest-frame Optical and UV Morphologies of Galaxies at $z=4-10$: First Phase of Inside-Out Galaxy Formation
by: Ono, Yoshiaki, et al.
Published: (2023)

Deciphering Gas Dynamics and Star Formation in a z=1.1 Main Sequence Spiral Galaxy with ALMA and JWST
by: Liu, Zhaoran, et al.
Published: (2024)

Galaxy populations in protoclusters at cosmic noon
by: Andrews, Moira, et al.
Published: (2024)

Do z>6 quasars reside in protoclusters?
by: Fontanot, Fabio, et al.
Published: (2025)

Cosmic Himalayas: The Highest Quasar Density Peak Identified in a 10,000 deg$^2$ Sky with Spatial Discrepancies between Galaxies, Quasars, and IGM HI
by: Liang, Yongming, et al.
Published: (2024)

Statistics for Galaxy Outflows at $z\sim 6-9$ with Imaging and Spectroscopic Signatures Identified with JWST/NIRCam and NIRSpec Data
by: Zhang, Yechi, et al.
Published: (2023)

Stellar- and AGN-Driven Outflows in JWST Galaxies at z=3-9: More Frequent, Wider Opening Angles, and Mostly Bounded
by: Xu, Yi, et al.
Published: (2023)

A massive quiescent galaxy in a group environment at $z=4.53$
by: Kakimoto, Takumi, et al.
Published: (2023)

SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z > 6 Quasar Host Galaxies using the JWST NIRSpec Fixed Slit
by: Phillips, Camryn L., et al.
Published: (2025)

Morphological Demographics of Galaxies at $z\sim 10-16$: Log-Normal Size Distribution and Exponential Profiles Consistent with the Disk Formation Scenario
by: Ono, Yoshiaki, et al.
Published: (2025)

The Growth of Galaxy Stellar Haloes Over $0.2 \leq z \leq 1.1$
by: Williams, Devin J., et al.
Published: (2024)

Probing the influence of the protocluster environment on galaxy morphology at z = 2.23
by: Golden-Marx, Emmet, et al.
Published: (2025)

MAMMOTH-Subaru IV. Large Scale Structure and Clustering Analysis of Ly$α$ Emitters and Ly$α$ Blobs at $z=2.2-2.3$
by: Zhang, Haibin, et al.
Published: (2023)

A UV-Luminous Galaxy at z=11 with Surprisingly Weak Star Formation Activity
by: Harikane, Yuichi, et al.
Published: (2026)

Not all protoclusters host evolved galaxies: Evidence for reduced environmental effects in a lower halo mass protocluster at $z = 7.66$
by: Witten, Callum, et al.
Published: (2025)

Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ Fields
by: Ito, Kei, et al.
Published: (2023)

JWST Measurements of Neutral Hydrogen Fractions and Ionized Bubble Sizes at $z=7-12$ Obtained with Ly$α$ Damping Wing Absorptions in 27 Bright Continuum Galaxies
by: Umeda, Hiroya, et al.
Published: (2023)

X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
by: Matsui, Suin, et al.
Published: (2023)