We propose a deep 100 ks observation of XLSSU J021744.1-034536, a galaxy clusterdiscovered by the XMM-LSS survey. The cluster was confirmed through optical andNIR imaging, and has 10-band photometric data indicating the very high redshiftof z=1.9. We obtained a high-significance detection of the Sunyaev-Zeldovicheffect of this system, confirming the presence of hot gas and providing anestimate of the cluster mass (1-2 10^14 Msun). The proposed observations willallow us to measure key properties of the intracluster medium, namely the gasmass, temperature and center-excised luminosity. The data will provide an anchorfor extending our understanding of cluster growth and scaling relations to highredshifts, and will enhance the cosmological power of the XMM-XXL survey.
Publications
The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field |Chen, C.-T. J., Brandt, W. N., et al. | MNRAS | 478-2132 | 2018 | 2018MNRAS.478.2132C | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.2132C
The XXL Survey. XVII. X-ray and Sunyaev-Zel.dovich properties of the redshift 2.0 galaxy cluster XLSSC 122 |Mantz, A. B., Abdulla, Z., et al. | A&A | 620-2 | 2018 | 2018A&A...620A...2M | http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...2M
Spectroscopic confirmation of a mature galaxy cluster at a redshift of 2 |Willis, J. P., Canning, R. E. A., et al. | Natur | 577-39 | 2020 | 2020Natur.577...39W | http://ui.adsabs.harvard.edu/#abs/2020Natur.577...39W
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies |Ojha, Vineet, Chand, Hum, et al. | ApJ | 896-95 | 2020 | 2020ApJ...896...95O | http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O
Implications of the Environments of Radio-detected Active Galactic Nuclei in a Complex Protostructure at z \\u223c 3.3 |Shen, Lu, Lemaux, Brian C., et al. | ApJ | 912-60 | 2021 | 2021ApJ...912...60S | http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...60S
The XXL Survey - XLVIII. X-ray follow-up of distant XXL clusters: masses, scaling relations, and AGN contamination |Duffy, R. T., Logan, C. H. A., et al. | MNRAS | 512-2525 | 2022 | 2022MNRAS.512.2525D | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.512.2525D
A fresh look at AGN spectral energy distribution fitting with the XMM-SERVS AGN sample |Marshall, Adam, Auger-Williams, Matthew W., et al. | MNRAS | 515-5617 | 2022 | 2022MNRAS.515.5617M | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.5617M
Detection of radio-AGN in dust-obscured galaxies using deep uGMRT radio continuum observations |Kayal, Abhijit, Singh, Veeresh, et al. | JApA | 43-84 | 2022 | 2022JApA...43...84K | http://ui.adsabs.harvard.edu/#abs/2022JApA...43...84K
Search and Characterization of Remnant Radio Galaxies in the XMM-LSS Deep Field |Dutta, Sushant, Singh, Veeresh, et al. | ApJ | 944-176 | 2023 | 2023ApJ...944..176D | http://ui.adsabs.harvard.edu/#abs/2023ApJ...944..176D
Observational properties of active galactic nucleus obscuration during the peak of accretion growth |Vijarnwannaluk, Bovornpratch, Akiyama, Masayuki, et al. | MNRAS | 529-3610 | 2024 | 2024MNRAS.529.3610V | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.3610V
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
2015-07-16T06:30:06Z/2015-07-17T12:06:46Z
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 Adam Mantz, 2016, 'Deep Observation of an SZ-confirmed XXL Galaxy Cluster at Redshift 1.9', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ju5lvjy
