Publications

Published Papers

  1. The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications, Cui et al., 2018, MNRAS, 480, 2898

  2. The Three Hundred Project: The Influence of Environment on Simulated Galaxy Properties, Wang et al., 2018, ApJ, 868,

  3. The Three Hundred Project: The evolution of galaxy cluster density profiles, Mostoghiu et al., 2019, MNRAS, 483, 3390

  4. THETHREEHUNDRED Project: ram pressure and gas content of haloes and subhaloes in the phase-space plane, Arthur et al., 2019, MNRAS, 484, 3968

  5. The Three Hundred Project: Correcting for the hydrostatic-equilibrium mass bias in X-ray and SZ surveys, Ansarifard et al., 2020, A&A, 634,

  6. The Three Hundred project: backsplash galaxies in simulations of clusters, Haggar et al., 2020, MNRAS, 492, 6074

  7. Mapping and characterization of cosmic filaments in galaxy cluster outskirts: strategies and forecasts for observations from simulations, Kuchner et al., 2020, MNRAS, 494, 5473

  8. The Three Hundred project: the stellar and gas profiles, Li et al., 2020, MNRAS, 495, 2930

  9. The Three Hundred project: shapes and radial alignment of satellite, infalling, and backsplash galaxies, Knebe et al., 2020, MNRAS, 495, 3002

  10. Constraining the cross-section of dark matter with giant radial arcs in galaxy clusters, Vega-Ferrero et al., 2021, MNRAS, 500, 247

  11. The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters, Haggar et al., 2021, MNRAS, 502, 1191

  12. The Three Hundred project: the gas disruption of infalling objects in cluster environments, Mostoghiu et al., 2021, MNRAS, 501, 5029

  13. The ThreeHundred: the structure and properties of cosmic filaments in the outskirts of galaxy clusters, Rost et al., 2021, MNRAS, 502, 714

  14. Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space, Kuchner et al., 2021, MNRAS, 503, 2065

  15. The Three Hundred project: quest of clusters of galaxies morphology and dynamical state through Zernike polynomials, Capalbo et al., 2021, MNRAS, 503, 6155

  16. The Three Hundred project: dynamical state of galaxy clusters and morphology from multiwavelength synthetic maps, De Luca et al., 2021, MNRAS, 504, 5383

  17. CLUMP-3D: the lack of non-thermal motions in galaxy cluster cores, Sayers et al., 2021, MNRAS, 505, 4338

  18. The Three Hundred Project: The stellar angular momentum evolution of cluster galaxies, Mostoghiu et al., 2021, A&A, 652,

  19. What to expect from dynamical modelling of cluster haloes - I. The information content of different dynamical tracers, Li et al., 2021, MNRAS, 505, 3907

  20. The thermalization of massive galaxy clusters, Sereno et al., 2021, MNRAS, 507, 5214

  21. Shocks in the stacked Sunyaev-Zel'dovich profiles of clusters - I. Analysis with the Three Hundred simulations, Baxter et al., 2021, MNRAS, 508, 1777

  22. Galaxy velocity bias in cosmological simulations: towards per cent-level calibration, Anbajagane et al., 2022, MNRAS, 510, 2980

  23. An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies, Kuchner et al., 2022, MNRAS, 510, 581

  24. Chameleon screening depends on the shape and structure of NFW halos, Tamosiunas et al., 2022, JCAP, 2022,

  25. 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

  26. Cosmic filaments delay quenching inside clusters, Kotecha et al., 2022, MNRAS, 512, 926

  27. The Three Hundred project: dissecting the Fundamental Plane of galaxy clusters up to z = 1, Díaz-García et al., 2022, MNRAS, 512, 1214

  28. Brightest cluster galaxies trace weak lensing mass bias and halo triaxiality in the three hundred project, Herbonnet et al., 2022, MNRAS, 513, 2178

  29. THE THREE HUNDRED project: Contrasting clusters galaxy density in hydrodynamical and dark matter only simulations, Jiménez Muñoz et al., 2022, EPJWC, 257,

  30. The Three Hundred-NIKA2 Sunyaev-Zeldovich Large Program twin samples: Synthetic clusters to support real observations, Paliwal et al., 2022, EPJWC, 257,

  31. Mass Estimation of Planck Galaxy Clusters using Deep Learning, de Andres et al., 2022, EPJWC, 257,

  32. Velocity dispersion vs cluster mass: A new scaling law with THE THREE HUNDRED clusters, Ferragamo et al., 2022, EPJWC, 257,

  33. THE THREE HUNDRED project: The GIZMO-SIMBA run, Cui et al., 2022, MNRAS, 514, 977

  34. The hydrostatic mass bias in THE THREE HUNDRED clusters, Gianfagna et al., 2022, EPJWC, 257,

  35. The THREEHUNDRED project: The effect of baryon processes at galaxy cluster scale, Cui et al., 2022, EPJWC, 257,

  36. Morphological analysis of SZ and X-ray maps of galaxy clusters with Zernike polynomials, Capalbo et al., 2022, EPJWC, 257,

  37. 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

  38. What to expect from dynamical modelling of cluster haloes - II. Investigating dynamical state indicators with Random Forest, Li et al., 2022, MNRAS, 514, 5890

  39. A stochastic model to reproduce the star formation history of individual galaxies in hydrodynamic simulations, Wang et al., 2022, MNRAS, 515, 3249

  40. THE THREE HUNDRED: cluster dynamical states and relaxation period, Zhang et al., 2022, MNRAS, 516, 26

  41. A deep learning approach to infer galaxy cluster masses from Planck Compton-y parameter maps, de Andres et al., 2022, NatAs, 6, 1325

  42. 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

  43. A multisimulation study of relativistic SZ temperature scalings in galaxy clusters and groups, Lee et al., 2022, MNRAS, 517, 5303

  44. 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

  45. A study of the hydrostatic mass bias dependence and evolution within The Three Hundred clusters, Gianfagna et al., 2023, MNRAS, 518, 4238

  46. 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

  47. The Three Hundred project: galaxy groups do not survive cluster infall, Haggar et al., 2023, MNRAS, 518, 1316

  48. 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,

  49. 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

  50. The Concentration-Mass relation of massive, dynamically relaxed galaxy clusters: agreement between observations and ΛCDM simulations, Darragh-Ford et al., 2023, MNRAS, 521, 790

  51. 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

  52. CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles, Bartalucci et al., 2023, A&A, 674,

  53. THE THREE HUNDRED Project: the evolution of physical baryon profiles, Li et al., 2023, MNRAS, 523, 1228

  54. Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters, Lokken et al., 2023, MNRAS, 523, 1346

  55. Diffuse radio emission from merger shocks in simulated galaxy clusters, Nuza et al., 2023, BAAA, 64, 166

  56. 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

  57. A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters, Meneghetti et al., 2023, A&A, 678,

  58. 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,

  59. The localization of galaxy groups in close proximity to galaxy clusters using cosmic web nodes, Cornwell et al., 2024, MNRAS, 527, 23

  60. The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters, Baxter et al., 2024, MNRAS, 527, 7847

  61. 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

  62. 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,

  63. Prospects for studying the mass and gas in protoclusters with future CMB observations, Gardner et al., 2024, OJAp, 7,

  64. 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

  65. CHEX-MATE: Characterization of the intra-cluster medium temperature distribution, Lovisari et al., 2024, A&A, 682,

  66. The Three Hundred: M<SUB>sub</SUB>-V<SUB>circ</SUB> relation, Srivastava et al., 2024, MNRAS, 528, 4451

  67. Characterising the intra-cluster light in The Three Hundred simulations, Contreras-Santos et al., 2024, A&A, 683,

  68. Identifying galaxy cluster mergers with deep neural networks using idealized Compton-y and X-ray maps, Arendt et al., 2024, MNRAS, 530, 20

  69. Intrinsic Mass–Richness Relation of Clusters from THE THREE HUNDRED Hydrodynamic Simulations, Chen et al., 2024, ApJ, 966,

  70. THE THREE HUNDRED: Contrasting cluster galaxy density in hydrodynamical and dark matter simulations, Jiménez Muñoz et al., 2024, A&A, 686,

  71. Impact of filaments on galaxy cluster properties in The Three Hundred simulation, Santoni et al., 2024, EPJWC, 293,

  72. 3D scaling laws and projection effects in The300-NIKA2 Sunyaev-Zeldovich Large Program Twin Samples, Paliwal et al., 2024, EPJWC, 293,

  73. Reconsidering the dynamical states of galaxy clusters using PCA and UMAP, Haggar et al., 2024, MNRAS, 532, 1031

  74. A Generative Model for Realistic Galaxy Cluster X-Ray Morphologies, Benyas et al., 2024, ApJ, 969,

Other publications

  1. The Three Hundred: $M_{sub}-V_{circ}$ relation, Srivastava et al., 2023, arXiv230906187S, ,

  2. Galaxy clusters morphology with Zernike polynomials: the first application on $\textit{Planck}$ Compton parameter maps, Capalbo et al., 2023, arXiv231007759C, ,

  3. The Effect of AGN Feedback on the Lyman-{\alpha} Forest Signature of Galaxy Protoclusters at z~2.3, Dong et al., 2024, arXiv240213568D, ,

  4. Generating Galaxy Clusters Mass Density Maps from Mock Multiview Images via Deep Learning, de Andres et al., 2024, arXiv240405400D, ,

  5. The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters, Santoni et al., 2024, arXiv240517239S, ,

More details and data can be found in the ADS libary.