We propose to follow up four distant galaxy clusters discovered by the XMM-LSSand XXL survey programs. In addition to being confirmed with optical and NIRspectroscopy or photometry, the presence of hot gas in each of these clustershas been confirmed through a significant detection of the Sunyaev-Zel dovichsignal with CARMA. Three of our targets have redshifts greater than 1, with oneof them at 1.5. Deeper XMM data will allow us to situate these high-redshiftclusters on X-ray and SZ scaling relations and provide key mass proxies,enhancing the cosmological power of the XXL survey and enabling a variety ofstudies of cluster evolution. We also request joint Chandra observations inorder to constrain and remove point-source contamination of the XMM signal for these faint clusters.
Publications
The XXL Survey. XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters |Koulouridis, E., Poggianti, B., et al. | A&A | 592-11 | 2016 | 2016A&A...592A..11K | http://ui.adsabs.harvard.edu/#abs/2016A&A...592A..11K
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
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
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
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
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
X-ray spectral properties of dust-obscured galaxies in the XMM-SERVS coverage of the XMM-LSS field |Kayal, Abhijit, Singh, Veeresh, | MNRAS | 531-830 | 2024 | 2024MNRAS.531..830K | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..830K
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
2014-06-29T04:28:48Z/2015-02-07T23:11:38Z
Version
PPS_NOT_AVAILABLE
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, 'Scaling Relations of Distant comma SZ-confirmed XXL Galaxy Clusters', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-2dfk7jf