:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Korkidis, Giorgos, Pavlidou, Vasiliki, Tassis, Konstantinos, Ntormousi, Evangelia, Tomaras, Theodore N., Kovlakas, Konstantinos
Formato:	Preprint
Publicado:	2019
Materias:	Cosmology and Nongalactic Astrophysics
Acceso en línea:	https://arxiv.org/abs/1912.08216
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

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

Mass scaling relations for dark halos from an analytic universal outer density profile
por: Korkidis, Giorgos, et al.
Publicado: (2024)

Searching for a signature of turnaround in galaxy clusters with convolutional neural networks
por: Triantafyllou, Nikolaos, et al.
Publicado: (2024)

Magnetising galaxies with cold inflows
por: Ledos, Nicolas, et al.
Publicado: (2024)

Getting the tiger by the tail: Probing the turnaround radius of structures with outer halo density profiles
por: Grammatikos, Kyriakos, et al.
Publicado: (2018)

Characterising galaxy cluster scaling relations as cosmic isotropy tracers using FLAMINGO simulations
por: He, Yujie, et al.
Publicado: (2025)

Galaxy clusters as probes of cosmic isotropy
por: Migkas, Konstantinos
Publicado: (2024)

Can the splashback radius be an observable boundary of galaxy clusters?
por: Lebeau, Théo, et al.
Publicado: (2024)

Dynamical friction and measurements of the splashback radius in galaxy clusters
por: O'Shea, Talia M., et al.
Publicado: (2024)

Constraining cosmological parameters using the splashback radius of galaxy clusters
por: Haggar, Roan, et al.
Publicado: (2024)

AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
por: Lesci, G. F., et al.
Publicado: (2026)

Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
por: Joshi, Jitendra, et al.
Publicado: (2025)

The splashback radius and the radial velocity profile of galaxy clusters in IllustrisTNG
por: Pizzardo, Michele, et al.
Publicado: (2023)

Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations
por: Towler, Imogen, et al.
Publicado: (2023)

AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
por: Giocoli, Carlo, et al.
Publicado: (2024)

From nuclear star clusters to Little Red Dots: black hole growth, mergers, and tidal disruptions
por: Kritos, Konstantinos, et al.
Publicado: (2025)

Impact of filaments on galaxy cluster properties in The Three Hundred simulation
por: Santoni, Sara, et al.
Publicado: (2023)

Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
por: Gallo, Stefano, et al.
Publicado: (2023)

Toward Black Hole Stars: supermassive black hole growth in nuclear clusters via stellar-object and gas accretion
por: Kritos, Konstantinos, et al.
Publicado: (2026)

Reconstructing spatially-varying multiplicative bias for Stage IV weak lensing galaxy surveys with a quadratic estimator
por: Tanidis, Konstantinos, et al.
Publicado: (2025)

The relation between the cool-core radius and the host galaxy clusters: thermodynamic properties and cluster mass
por: Ng, FanLam, et al.
Publicado: (2023)

Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
por: Fontanot, Fabio, et al.
Publicado: (2024)

Hydrostatic mass bias for galaxy groups and clusters in the FLAMINGO simulations
por: Braspenning, Joey, et al.
Publicado: (2024)

Suppressing the sample variance of DESI-like galaxy clustering with fast simulations
por: Ding, Z., et al.
Publicado: (2024)

Diffuse radio emission from merger shocks in simulated galaxy clusters
por: Nuza, Sebastián E.
Publicado: (2024)

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

Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code
por: Kritos, Konstantinos, et al.
Publicado: (2022)

Bridging observations and simulations: a machine learning approach to galaxy clusters
por: Gatuzz, Efrain
Publicado: (2025)

Predicting intermediate-mass black hole formation in star clusters with machine learning
por: Kritos, Konstantinos, et al.
Publicado: (2026)

The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
por: Muñoz, A. Jiménez, et al.
Publicado: (2023)

The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
por: Corasaniti, P. S., et al.
Publicado: (2025)

Extracting cosmological information from the abundance of galaxy clusters with simulation-based inference
por: Zubeldia, Íñigo, et al.
Publicado: (2025)

Direct N-body simulations of rotating and extremely massive Population III star clusters
por: Wu, Kai, et al.
Publicado: (2026)

An N-body/hydrodynamical simulation study of the merging cluster El Gordo: A compelling case for self-interacting dark matter?
por: Valdarnini, R.
Publicado: (2023)

Redshift Drift fluctuations from N-body simulations
por: Bessa, Pedro, et al.
Publicado: (2024)

The full iron budget in simulated galaxy clusters: The chemistry between gas and stars
por: Biffi, Veronica, et al.
Publicado: (2025)

Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters
por: Dacunha, Tara, et al.
Publicado: (2025)

The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
por: Beordo, William, et al.
Publicado: (2025)

Cosmological simulation of a radio synchrotron bridge between pre-merging galaxy clusters
por: Nishiwaki, Kosuke, et al.
Publicado: (2026)

Unifying cluster and galaxy cosmology analyses using the galaxy-halo connection
por: Cao, Shulei, et al.
Publicado: (2026)