The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications, Cui et al., 2018, MNRAS, 480, 2898
The Three Hundred Project: The Influence of Environment on Simulated Galaxy Properties, Wang et al., 2018, ApJ, 868,
The Three Hundred Project: The evolution of galaxy cluster density profiles, Mostoghiu et al., 2019, MNRAS, 483, 3390
THETHREEHUNDRED Project: ram pressure and gas content of haloes and subhaloes in the phase-space plane, Arthur et al., 2019, MNRAS, 484, 3968
The Three Hundred Project: Correcting for the hydrostatic-equilibrium mass bias in X-ray and SZ surveys, Ansarifard et al., 2020, A&A, 634,
The Three Hundred project: backsplash galaxies in simulations of clusters, Haggar et al., 2020, MNRAS, 492, 6074
Mapping and characterization of cosmic filaments in galaxy cluster outskirts: strategies and forecasts for observations from simulations, Kuchner et al., 2020, MNRAS, 494, 5473
The Three Hundred project: shapes and radial alignment of satellite, infalling, and backsplash galaxies, Knebe et al., 2020, MNRAS, 495, 3002
The Three Hundred project: the stellar and gas profiles, Li et al., 2020, MNRAS, 495, 2930
Constraining the cross-section of dark matter with giant radial arcs in galaxy clusters, Vega-Ferrero et al., 2021, MNRAS, 500, 247
The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters, Haggar et al., 2021, MNRAS, 502, 1191
The Three Hundred project: the gas disruption of infalling objects in cluster environments, Mostoghiu et al., 2021, MNRAS, 501, 5029
The ThreeHundred: the structure and properties of cosmic filaments in the outskirts of galaxy clusters, Rost et al., 2021, MNRAS, 502, 714
Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space, Kuchner et al., 2021, MNRAS, 503, 2065
The Three Hundred project: quest of clusters of galaxies morphology and dynamical state through Zernike polynomials, Capalbo et al., 2021, MNRAS, 503, 6155
The Three Hundred project: dynamical state of galaxy clusters and morphology from multiwavelength synthetic maps, De Luca et al., 2021, MNRAS, 504, 5383
CLUMP-3D: the lack of non-thermal motions in galaxy cluster cores, Sayers et al., 2021, MNRAS, 505, 4338
The Three Hundred Project: The stellar angular momentum evolution of cluster galaxies, Mostoghiu et al., 2021, A&A, 652,
What to expect from dynamical modelling of cluster haloes - I. The information content of different dynamical tracers, Li et al., 2021, MNRAS, 505, 3907
The thermalization of massive galaxy clusters, Sereno et al., 2021, MNRAS, 507, 5214
Shocks in the stacked Sunyaev-Zel'dovich profiles of clusters - I. Analysis with the Three Hundred simulations, Baxter et al., 2021, MNRAS, 508, 1777
An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies, Kuchner et al., 2022, MNRAS, 510, 581
Galaxy velocity bias in cosmological simulations: towards per cent-level calibration, Anbajagane et al., 2022, MNRAS, 510, 2980
Chameleon screening depends on the shape and structure of NFW halos, Tamosiunas et al., 2022, JCAP, 2022,
The three hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies, Contreras-Santos et al., 2022, MNRAS, 511, 2897
Cosmic filaments delay quenching inside clusters, Kotecha et al., 2022, MNRAS, 512, 926
The Three Hundred project: dissecting the Fundamental Plane of galaxy clusters up to z = 1, Díaz-García et al., 2022, MNRAS, 512, 1214
Brightest cluster galaxies trace weak lensing mass bias and halo triaxiality in the three hundred project, Herbonnet et al., 2022, MNRAS, 513, 2178
The hydrostatic mass bias in THE THREE HUNDRED clusters, Gianfagna et al., 2022, EPJWC, 257,
Morphological analysis of SZ and X-ray maps of galaxy clusters with Zernike polynomials, Capalbo et al., 2022, EPJWC, 257,
The THREEHUNDRED project: The effect of baryon processes at galaxy cluster scale, Cui et al., 2022, EPJWC, 257,
Mass Estimation of Planck Galaxy Clusters using Deep Learning, de Andres et al., 2022, EPJWC, 257,
Velocity dispersion vs cluster mass: A new scaling law with THE THREE HUNDRED clusters, Ferragamo et al., 2022, EPJWC, 257,
The Three Hundred-NIKA2 Sunyaev-Zeldovich Large Program twin samples: Synthetic clusters to support real observations, Paliwal et al., 2022, EPJWC, 257,
THE THREE HUNDRED project: Contrasting clusters galaxy density in hydrodynamical and dark matter only simulations, Jiménez Muñoz et al., 2022, EPJWC, 257,
THE THREE HUNDRED project: The GIZMO-SIMBA run, Cui et al., 2022, MNRAS, 514, 977
What to expect from dynamical modelling of cluster haloes - II. Investigating dynamical state indicators with Random Forest, Li et al., 2022, MNRAS, 514, 5890
Shocks in the stacked Sunyaev-Zel'dovich profiles of clusters II: Measurements from SPT-SZ + Planck Compton-y map, Anbajagane et al., 2022, MNRAS, 514, 1645
A stochastic model to reproduce the star formation history of individual galaxies in hydrodynamic simulations, Wang et al., 2022, MNRAS, 515, 3249
THE THREE HUNDRED: cluster dynamical states and relaxation period, Zhang et al., 2022, MNRAS, 516, 26
A deep learning approach to infer galaxy cluster masses from Planck Compton-y parameter maps, de Andres et al., 2022, NatAs, 6, 1325
A multisimulation study of relativistic SZ temperature scalings in galaxy clusters and groups, Lee et al., 2022, MNRAS, 517, 5303
Forecasting the success of the WEAVE Wide-Field Cluster Survey on the extraction of the cosmic web filaments around galaxy clusters, Cornwell et al., 2022, MNRAS, 517, 1678
The Three Hundred project: galaxy groups do not survive cluster infall, Haggar et al., 2023, MNRAS, 518, 1316
The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters, Hough et al., 2023, MNRAS, 518, 2398
A study of the hydrostatic mass bias dependence and evolution within The Three Hundred clusters, Gianfagna et al., 2023, MNRAS, 518, 4238
Machine learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations, de Andres et al., 2023, MNRAS, 518, 111
The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 ≤ z ≤ 0.60 and 4 × 10<SUP>14</SUP> M <SUB>⊙</SUB> ≤ M <SUB>500</SUB> ≤ 30 × 10<SUP>14</SUP> M <SUB>⊙</SUB>, Sayers et al., 2023, ApJ, 944,
THE THREE HUNDRED project: a machine learning method to infer clusters of galaxy mass radial profiles from mock Sunyaev-Zel'dovich maps, Ferragamo et al., 2023, MNRAS, 520, 4000
The Concentration-Mass relation of massive, dynamically relaxed galaxy clusters: agreement between observations and ΛCDM simulations, Darragh-Ford et al., 2023, MNRAS, 521, 790
CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles, Bartalucci et al., 2023, A&A, 674,
Galaxy pairs in THE THREE HUNDRED simulations II: studying bound ones and identifying them via machine learning, Contreras-Santos et al., 2023, MNRAS, 522, 1270
Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters, Lokken et al., 2023, MNRAS, 523, 1346
THE THREE HUNDRED Project: the evolution of physical baryon profiles, Li et al., 2023, MNRAS, 523, 1228
Diffuse radio emission from merger shocks in simulated galaxy clusters, Nuza et al., 2023, BAAA, 64, 166
The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey, Cornwell et al., 2023, MNRAS, 524, 2148
A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters, Meneghetti et al., 2023, A&A, 678,
CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles, Iqbal et al., 2023, A&A, 679,
The three hundred project: thermodynamical properties, shocks, and gas dynamics in simulated galaxy cluster filaments and their surroundings, Rost et al., 2024, MNRAS, 527, 1301
Euclid preparation. XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations, Euclid Collaboration et al., 2024, A&A, 681,
Prospects for studying the mass and gas in protoclusters with future CMB observations, Gardner et al., 2024, OJAp, 7,
The localization of galaxy groups in close proximity to galaxy clusters using cosmic web nodes, Cornwell et al., 2024, MNRAS, 527, 23
The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters, Baxter et al., 2024, MNRAS, 527, 7847
CHEX-MATE: Characterization of the intra-cluster medium temperature distribution, Lovisari et al., 2024, A&A, 682,
The three hundred project: mapping the matter distribution in galaxy clusters via deep learning from multiview simulated observations, de Andres et al., 2024, MNRAS, 528, 1517
The Three Hundred: M<SUB>sub</SUB>-V<SUB>circ</SUB> relation, Srivastava et al., 2024, MNRAS, 528, 4451
Characterising the intra-cluster light in The Three Hundred simulations, Contreras-Santos et al., 2024, A&A, 683,
Identifying galaxy cluster mergers with deep neural networks using idealized Compton-y and X-ray maps, Arendt et al., 2024, MNRAS, 530, 20
Intrinsic Mass–Richness Relation of Clusters from THE THREE HUNDRED Hydrodynamic Simulations, Chen et al., 2024, ApJ, 966,
Impact of filaments on galaxy cluster properties in The Three Hundred simulation, Santoni et al., 2024, EPJWC, 293,
3D scaling laws and projection effects in The300-NIKA2 Sunyaev-Zeldovich Large Program Twin Samples, Paliwal et al., 2024, EPJWC, 293,
THE THREE HUNDRED: Contrasting cluster galaxy density in hydrodynamical and dark matter simulations, Jiménez Muñoz et al., 2024, A&A, 686,
A Generative Model for Realistic Galaxy Cluster X-Ray Morphologies, Benyas et al., 2024, ApJ, 969,
Reconsidering the dynamical states of galaxy clusters using PCA and UMAP, Haggar et al., 2024, MNRAS, 532, 1031
The effect of AGN feedback on the Lyman-α forest signature of galaxy protoclusters at z 2.3, Dong et al., 2024, MNRAS, 532, 4876
The Three Hundred project: Radio luminosity evolution from merger-induced shock fronts in simulated galaxy clusters, Nuza et al., 2024, A&A, 690,
The Three Hundred: The existence of massive dark matter-deficient satellite galaxies in cosmological simulations, Contreras-Santos et al., 2024, A&A, 690,
Galaxy clusters morphology with Zernike polynomials: the first application on $\textit{Planck}$ Compton parameter maps, Capalbo et al., 2023, arXiv231007759C, ,
Generating Galaxy Clusters Mass Density Maps from Mock Multiview Images via Deep Learning, de Andres et al., 2024, arXiv240405400D, ,
The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters, Santoni et al., 2024, arXiv240517239S, ,
Deep Learning generated observations of galaxy clusters from dark-matter-only simulations, Caro et al., 2024, arXiv241004229C, ,
Inference of morphology and dynamical state of nearby $Planck$-SZ galaxy clusters with Zernike polynomials, Capalbo et al., 2024, arXiv241013929C, ,
The Atacama Cosmology Telescope: a census of bridges between galaxy clusters, Isopi et al., 2024, arXiv241014404I, ,
Stellar stripping efficiencies of satellites in numerical simulations: the effect of resolution, satellite properties and numerical disruption, Martin et al., 2024, arXiv241019292M, ,
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