Imagen de Portada

Beyond Linear Bias Expansions for AbacusSummit Halos at z = 8

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Boone, Kyle K., Eisenstein, Daniel J.
Formato:	Preprint
Publicado:	2026
Materias:	Cosmology and Nongalactic Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

The DESI One-Percent survey: exploring the Halo Occupation Distribution of Emission Line Galaxies with AbacusSummit simulations
por: Rocher, Antoine, et al.
Publicado: (2023)

Measuring and unbiasing the BAO shift in the Lyman-Alpha forest with AbacusSummit
por: Hadzhiyska, Boryana, et al.
Publicado: (2025)

AbacusPNG: A modest set of simulations of local-type primordial non-Gaussianity in the DESI era
por: Hadzhiyska, Boryana, et al.
Publicado: (2024)

An Improved Fit for Linear Halo Bias at High Redshift
por: Wang, Kuan, et al.
Publicado: (2026)

Monopole Fluctuations in Galaxy Surveys
por: Yoo, Jaiyul, et al.
Publicado: (2024)

Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum
por: Miller, Kyle, et al.
Publicado: (2025)

Non-Separable Halo Bias from High-Redshift Galaxy Clustering
por: Mons, Emy, et al.
Publicado: (2025)

Reversing Arrested Development: A New Method to Address Halo Assembly Bias
por: Smith, William, et al.
Publicado: (2024)

Probing primordial non-Gaussianity by reconstructing the initial conditions
por: Chen, Xinyi, et al.
Publicado: (2024)

Optimal intrinsic alignment estimators in the presence of redshift-space distortions
por: Lamman, Claire, et al.
Publicado: (2025)

Discovery of a $z \sim 0.8$ Ultra Steep Spectrum Radio Halo in the MeerKAT-South Pole Telescope Survey
por: Magolego, Isaac S., et al.
Publicado: (2025)

Hubble Expansion Signature on Simulated Halo Density Profiles: A Path to Observing the Turnaround Radius
por: Korkidis, Giorgos, et al.
Publicado: (2024)

Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
por: Bartlett, Deaglan J., et al.
Publicado: (2024)

Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
por: Kim, Yigon, et al.
Publicado: (2025)

AtLAST -- Determination of Halo Mass Density Profiles at kpc Scales through Magnification Bias
por: González-Nuevo, Joaquín, et al.
Publicado: (2025)

The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
por: Wang, Kuan, et al.
Publicado: (2023)

EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\gtrsim6$
por: Eilers, Anna-Christina, et al.
Publicado: (2024)

MUSE-ALMA Haloes XIII. Molecular gas in $z \sim 0.5$ HI-selected galaxies
por: Bollo, Victoria, et al.
Publicado: (2026)

Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
por: Low, Ryan, et al.
Publicado: (2025)

Core Collapse Beyond the Fluid Approximation: The Late Evolution of Self-Interacting Dark Matter Halos
por: Gurian, James, et al.
Publicado: (2025)

Ellipticities of Galaxy Cluster Halos from Halo-Shear-Shear Correlations
por: Liu, Zhenjie, et al.
Publicado: (2024)

Group Therapy for Halos: Advancing Halo Mass Estimation for Galaxy Groups
por: Van Kempen, Welsey, et al.
Publicado: (2025)

The Halo Occupation Distribution Modeling of the X-ray-selected AGNs at 0.6 < z < 2.6 in the COSMOS field
por: Ikeda, Hiroyuki, et al.
Publicado: (2025)

CSST Cosmological Emulator III: Hybrid Lagrangian Bias Expansion Emulation of Galaxy Clustering
por: Zhou, Shuren, et al.
Publicado: (2025)

Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias
por: Abdelaziz, Mariam, et al.
Publicado: (2026)

Predicting Halo Formation Time Using Machine Learning
por: Srivastava, Atulit, et al.
Publicado: (2025)

Beyond MACS: Physical properties of extremely X-ray luminous clusters at $z > 0.5$
por: Ebeling, H., et al.
Publicado: (2024)

On the Outskirts of Dark Matter Haloes
por: Chen, Alice, et al.
Publicado: (2022)

The Density Profile of Dynamical Halos
por: Shields, Tristen, et al.
Publicado: (2025)

Discovery of Diffuse Radio Emission in a Massive z=1.709 Cool Core Cluster: A Candidate Radio Mini-Halo
por: Hlavacek-Larrondo, Julie, et al.
Publicado: (2025)

Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions
por: Buisman, Jim, et al.
Publicado: (2025)

An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
por: Sullivan, James M., et al.
Publicado: (2021)

Beyond $Λ$CDM with $f(z)$CDM: criticalities and solutions of Padé Cosmography
por: Petreca, Alexandra T., et al.
Publicado: (2023)

Halo Mergers Enhance the Growth of Massive Black Hole Seeds
por: Prole, Lewis R., et al.
Publicado: (2024)

HaloFlow II: Robust Galaxy Halo Mass Inference with Domain Adaptation
por: Garuda, Nikhil, et al.
Publicado: (2026)

Reconstruction of Dark Matter and Baryon Density From Galaxies: A Comparison of Linear, Halo Model and Machine Learning-Based Methods
por: Krywonos, Jordan, et al.
Publicado: (2025)

Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1
por: Mertens, F. G., et al.
Publicado: (2025)

Halo asymmetry in the modelling of galaxy clustering
por: Durkalec, Anna, et al.
Publicado: (2024)

Halo mass functions at high redshift
por: O'Brennan, Hannah, et al.
Publicado: (2024)

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR
por: Ghara, R., et al.
Publicado: (2025)