Publications |
- Probing the evolution of the substructure frequency in galaxy clusters up to z virgul 1 |Weissmann, A., Bohringer, H., | A&A | 555-147 | 2013 | 2013A&A...555A.147W | http://ui.adsabs.harvard.edu/#abs/2013A&A...555A.147W
- Warm--hot baryons comprise 5--10 per cent of filaments in the cosmic web |Eckert, Dominique, Jauzac, Mathilde, et al. | Natur | 528-105 | 2015 | 2015Natur.528..105E | http://ui.adsabs.harvard.edu/#abs/2015Natur.528..105E
- Frontier Fields: Subaru Weak-Lensing Analysis of the Merging Galaxy Cluster A2744 |Medezinski, Elinor, Umetsu, Keiichi, et al. | ApJ | 817-24 | 2016 | 2016ApJ...817...24M | http://ui.adsabs.harvard.edu/#abs/2016ApJ...817...24M
- A shock front at the radio relic of Abell 2744 |Eckert, D., Jauzac, M., et al. | MNRAS | 461-1302 | 2016 | 2016MNRAS.461.1302E | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461.1302E
- The extraordinary amount of substructure in the Hubble Frontier Fields cluster Abell 2744 |Jauzac, M., Eckert, D., et al. | MNRAS | 463-3876 | 2016 | 2016MNRAS.463.3876J | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.3876J
- A study of halo and relic radio emission in merging clusters using the Murchison Widefield Array |George, L. T., Dwarakanath, K. S., et al. | MNRAS | 467-936 | 2017 | 2017MNRAS.467..936G | http://ui.adsabs.harvard.edu/#abs/2017MNRAS.467..936G
- X-Ray Morphological Analysis of the Planck ESZ Clusters |Lovisari, Lorenzo, Forman, William R., et al. | ApJ | 846-51 | 2017 | 2017ApJ...846...51L | http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L
- Search for the warm-hot intergalactic medium around A 2744 using Suzaku |Hattori, Shiho, Ota, Naomi, et al. | PASJ | 69-39 | 2017 | 2017PASJ...69...39H | http://ui.adsabs.harvard.edu/#abs/2017PASJ...69...39H
- Diffuse Radio Emission from Galaxy Clusters |van Weeren, R. J., de Gasperin, F., et al. | SSRv | 215-16 | 2019 | 2019SSRv..215...16V | http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...16V
- Shock acceleration efficiency in radio relics |Botteon, A., Brunetti, G., et al. | A&A | 634-64 | 2020 | 2020A&A...634A..64B | http://ui.adsabs.harvard.edu/#abs/2020A&A...634A..64B
- X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton |Lovisari, Lorenzo, Schellenberger, Gerrit, et al. | ApJ | 892-102 | 2020 | 2020ApJ...892..102L | http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L
- The BUFFALO HST Survey |Steinhardt, Charles L., Jauzac, Mathilde, et al. | ApJS | 247-64 | 2020 | 2020ApJS..247...64S | http://ui.adsabs.harvard.edu/#abs/2020ApJS..247...64S
- Comparing different mass estimators for a large subsample of the Planck-ESZ clusters |Lovisari, L., Ettori, S., et al. | A&A | 644-78 | 2020 | 2020A&A...644A..78L | http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L
- The thermalization of massive galaxy clusters |Sereno, Mauro, Lovisari, Lorenzo, et al. | MNRAS | 507-5214 | 2021 | 2021MNRAS.507.5214S | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S
- Classification of 4XMM-DR9 sources by machine learning |Zhang, Yanxia, Zhao, Yongheng, | MNRAS | 503-5263 | 2021 | 2021MNRAS.503.5263Z | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z
- The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview |CHEX-MATE Collaboration, Arnaud, M., et al. | A&A | 650-104 | 2021 | 2021A&A...650A.104C | http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.104C
- CHEX-MATE: Morphological analysis of the sample |Campitiello, M. G., Ettori, S., et al. | A&A | 665-117 | 2022 | 2022A&A...665A.117C | http://ui.adsabs.harvard.edu/#abs/2022A&A...665A.117C
- Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters |Wicker, R., Douspis, M., et al. | A&A | 674-48 | 2023 | 2023A&A...674A..48W | http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W
- CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles |Bartalucci, I., Molendi, S., et al. | A&A | 674-179 | 2023 | 2023A&A...674A.179B | http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.179B
- CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters |Bourdin, H., De Luca, F., et al. | A&A | 678-181 | 2023 | 2023A&A...678A.181B | http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.181B
- Pressure profiles of distant Galaxy clusters with Planck-SPT data |Oppizzi, Filippo, De Luca, Federico, et al. | EPJWC | 257-00035 | 2022 | 2022EPJWC.25700035O | http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700035O
- CHEX-MATE: Characterization of the intra-cluster medium temperature distribution |Lovisari, L., Ettori, S., et al. | A&A | 682-A45 | 2024 | 2024A&A...682A..45L | http://ui.adsabs.harvard.edu/#abs/2024A&A...682A..45L
- From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources |Rodriguez, Antonio C., | PASP | 136-054201 | 2024 | 2024PASP..136e4201R | http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
- Robust constraints on feebly interacting particles using XMM-Newton |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
- Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
- Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints |De la Torre Luque, Pedro, Balaji, Shyam, | ApJ | 968-46 | 2024 | 2024ApJ...968...46D | http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
|
Keywords |
"sub clumps", "cluster core", "data proprietary", "frontier field cluster", "XMM", "massive cluster merger", "scale matter distribution", "complex merging taking", "xmm frontier", "pandora cluster", "hydrostatic mass", "deep xmm", "data set", "virial radius", "thermodynamic properties", "HST" |