The distribution of dark matter, baryons, and stars in a cluster gravitationalpotential is a fundamental prediction of large-scale structure formation. Wehave 524 orbits of HST imaging together with Subaru and VLT spectroscopy tomeasure the strong and weak lensing properties of 20 relaxed and 5high-magnification galaxy clusters (z = 0.18 - 0.90, Tgas > 5 keV). Observingthe last 3 relaxed clusters with good visibility lacking XMM data will permituniform joint Xray/lensing/SZ analysis for 17 of the relaxed systems to advanceour understanding of the shapes and concentrations of the mass profiles,providing precise observational benchmarks for baryonic and dark matterdistributions over a range of redshifts.
Publications
Scaling Relations and X-Ray Properties of Moderate-luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton |Connor, Thomas, Donahue, Megan, et al. | ApJ | 794-48 | 2014 | 2014ApJ...794...48C | http://ui.adsabs.harvard.edu/#abs/2014ApJ...794...48C
High angular resolution Sunyaev-Zel.dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis |Adam, R., Comis, B., et al. | A&A | 586-122 | 2016 | 2016A&A...586A.122A | http://ui.adsabs.harvard.edu/#abs/2016A&A...586A.122A
LoCuSS: pre-processing in galaxy groups falling into massive galaxy clusters at z = 0.2 |Bianconi, M., Smith, G. P., et al. | MNRAS | 473-79 | 2018 | 2018MNRAS.473L..79B | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473L..79B
Thermodynamic profiles of galaxy clusters from a joint X-ray/SZ analysis |Shitanishi, Jennifer A., Pierpaoli, Elena, et al. | MNRAS | 481-749 | 2018 | 2018MNRAS.481..749S | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481..749S
Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects. A Millimetre/Submillimetre Probe of the Warm and Hot Universe |Mroczkowski, Tony, Nagai, Daisuke, et al. | SSRv | 215-17 | 2019 | 2019SSRv..215...17M | http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...17M
The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin |Bhargava, S., Giles, P. A., et al. | MNRAS | 497-656 | 2020 | 2020MNRAS.497..656B | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B
The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview |Botteon, A., Shimwell, T. W., et al. | A&A | 660-78 | 2022 | 2022A&A...660A..78B | http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B
The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium |Zhang, X., Simionescu, A., et al. | A&A | 672-42 | 2023 | 2023A&A...672A..42Z | http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z
The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models |Cassano, R., Cuciti, V., et al. | A&A | 672-43 | 2023 | 2023A&A...672A..43C | http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C
The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
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
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2013-08-22T22:03:38Z/2014-02-09T14:25:01Z
Version
17.56_20190403_1200
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Dr Megan Donahue, 2015, 'Baryons and Dark Matter in Hubble Treasury Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dxd2r3y
