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Bibliografische gegevens
Hoofdauteurs:	Chuang, Yao-Tsung, Okumura, Teppei, Nishimichi, Takahiro
Formaat:	Preprint
Gepubliceerd in:	2026
Onderwerpen:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Online toegang:	https://arxiv.org/abs/2602.04485
Tags:	Voeg label toe Geen labels, Wees de eerste die dit record labelt!

Gelijkaardige items

Nonlinear redshift space distortion in halo ellipticity correlations: Analytical model and N-body simulations
door: Okumura, Teppei, et al.
Gepubliceerd in: (2023)

Mock Observatory: two thousand lightcone mock catalogues of luminous red galaxies from the Hyper Suprime-Cam Survey for the cosmological large-scale analysis
door: Ishikawa, Shogo, et al.
Gepubliceerd in: (2023)

SHAPE: cosmology with cluster halo intrinsic alignments from subhalo distributions
door: Ishikawa, Shogo, et al.
Gepubliceerd in: (2025)

First confirmation of anisotropic halo bias from statistically anisotropic matter distributions
door: Masaki, Shogo, et al.
Gepubliceerd in: (2024)

Constraining cosmology with N-body simulations for future spectroscopic galaxy surveys at $2\leq z\leq 3$
door: Pu, Sy-Yun, et al.
Gepubliceerd in: (2024)

Clustering of emission line galaxies with IllustrisTNG -- II. cosmology challenge with anisotropic correlation functions and ELG-halo connections
door: Osato, Ken, et al.
Gepubliceerd in: (2026)

Inner structure of cold and warm dark matter halos from particle dynamics
door: Enomoto, Yohsuke, et al.
Gepubliceerd in: (2024)

Evidence for Intrinsic Galaxy Alignments in Ellipticity Autocorrelations out to $100 h^{-1}\textrm{Mpc}$ from SDSS Galaxies with DESI Imaging
door: Okumura, Teppei
Gepubliceerd in: (2025)

A new constraint on galaxy-halo connections of [O II] emitters via HOD modelling with angular clustering and luminosity functions from the Subaru HSC survey
door: Ishikawa, Shogo, et al.
Gepubliceerd in: (2024)

Galaxy Spin Alignment with Tidal Fields in the SDSS-IV MaNGA Survey
door: Moon, Jun-Sung, et al.
Gepubliceerd in: (2025)

Intrinsic Alignments and Spin Correlations of [OII] Emitters at $z=1.2$ and $z=1.5$ from HSC Narrow-band Survey
door: Tonegawa, Motonari, et al.
Gepubliceerd in: (2024)

Extracting parity-violating gravitational waves from projected tidal force tensor in three dimensions
door: Okumura, Teppei, et al.
Gepubliceerd in: (2024)

Probing the spatial and velocity anisotropies in stellar halos from the Aquarius simulations
door: Mondal, Amit, et al.
Gepubliceerd in: (2023)

Spin speed correlations and the evolution of galaxy-halo systems
door: Sheng, Ming-Jie, et al.
Gepubliceerd in: (2023)

Spatial and velocity anisotropies of stellar halos across cosmic web environments: Insights from IllustrisTNG simulation
door: Mondal, Amit, et al.
Gepubliceerd in: (2025)

Large-scale dual AGN in large-scale cosmological hydrodynamical simulations
door: Puerto-Sánchez, Clara, et al.
Gepubliceerd in: (2024)

High-redshift halo-galaxy connection via constrained simulations
door: Nusser, Adi
Gepubliceerd in: (2024)

On the impact of baryons on the halo mass function, bias, and cluster cosmology
door: Castro, Tiago, et al.
Gepubliceerd in: (2020)

Efficient hybrid technique for generating sub-grid haloes in reionization simulations
door: Barsode, Ankur, et al.
Gepubliceerd in: (2024)

Cosmological inference with halo clustering reconstructed from the redshift-space galaxy distribution
door: Hada, Ryuichiro, et al.
Gepubliceerd in: (2026)

The Intrinsic Alignment of Galaxy Clusters and Impact of Projection Effects
door: Shi, Jingjing, et al.
Gepubliceerd in: (2023)

How does the velocity anisotropy of halo stars, dark matter and satellite galaxies depend on host halo properties?
door: He, Jiaxin, et al.
Gepubliceerd in: (2024)

Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
door: Yesuf, Hassen M., et al.
Gepubliceerd in: (2026)

The impact of baryons on weak lensing statistics as a function of halo mass and radius
door: Lee, Max E., et al.
Gepubliceerd in: (2026)

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass
door: Shankar, Francesco, et al.
Gepubliceerd in: (2025)

Zooming by in the CARPoolGP lane: new CAMELS-TNG simulations of zoomed-in massive halos
door: Lee, Max E., et al.
Gepubliceerd in: (2024)

A universal scaling relation incorporating the cusp-to-core transition of dark matter haloes
door: Kaneda, Yuka, et al.
Gepubliceerd in: (2024)

Exploring gas thermodynamics around galaxies from the Sunyaev-Zel'dovich effects: impact of galaxy-halo connection, 2D projection and velocity field
door: Kadir, Sadaf, et al.
Gepubliceerd in: (2026)

Tomographic halo model of the unWISE-Blue galaxies using cross-correlations with BOSS CMASS galaxies
door: Krolewski, Alex, et al.
Gepubliceerd in: (2025)

Characterising ultra-high-redshift dark matter halo demographics and assembly histories with the GUREFT simulations
door: Yung, L. Y. Aaron, et al.
Gepubliceerd in: (2023)

Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
door: Li, Shun-Sheng, et al.
Gepubliceerd in: (2024)

The impact of galaxy bias on cross-correlation tomography
door: Maleubre, Sara, et al.
Gepubliceerd in: (2025)

EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
door: Wang, Yunchong, et al.
Gepubliceerd in: (2024)

Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
door: Mountrichas, G., et al.
Gepubliceerd in: (2026)

Evolution of Massive Red Galaxies in Clusters from z=1.0 to z=0.3
door: Lin, Yen-Ting, et al.
Gepubliceerd in: (2025)

The cusp-halo relation
door: Delos, M. Sten
Gepubliceerd in: (2025)

Quadratic shape biases in three-dimensional halo intrinsic alignments
door: Akitsu, Kazuyuki, et al.
Gepubliceerd in: (2023)

Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
door: Wang, Kai, et al.
Gepubliceerd in: (2023)

Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
door: Jun, Rui Lan, et al.
Gepubliceerd in: (2025)

Establishing HI mass v.s. stellar mass and halo mass scaling relations using an abundance matching method
door: Lu, Yi, et al.
Gepubliceerd in: (2024)