(Abridged) The South Pole Telescope (SPT) galaxy cluster survey identified viathe Sunyaev-Zel.dovich (SZ) effect 158 massive clusters from its initial 720deg2 area. We are proposing to combine XMM-Newton, SPT, and weak lensingmeasurements for a sample of 20 intermediate redshift (0.3<z<0.5) uniformlyselected by their SPT detection significance from 560 deg2 survey area. Theseclusters will also have ground-based observations weak lensing measurements andin some cases also dynamical masses. Here we propose to complete the X-rayfollow-up of the intermediate redshift calibration sample to uniform sensitivityand selection by observing the last 4 clusters without X-ray data andre-observing 4 clusters strongly affected by soft proton flaring.
X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton |Bulbul, Esra, Chiu, I.-Non, et al. | ApJ | 871-50 | 2019 | 2019ApJ...871...50B | http://ui.adsabs.harvard.edu/#abs/2019ApJ...871...50B
Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy - II. The X-ray luminosity-mass relation |Capasso, R., Mohr, J. J., et al. | MNRAS | 494-2736 | 2020 | 2020MNRAS.494.2736C | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.2736C
Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z \\u223c 1 |Gupta, N., Pannella, M., et al. | MNRAS | 494-1705 | 2020 | 2020MNRAS.494.1705G | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.1705G
A joint SZ-X-ray-optical analysis of the dynamical state of 288 massive galaxy clusters |Zenteno, A., Hern\\u00e1ndez-Lang, D., et al. | MNRAS | 495-705 | 2020 | 2020MNRAS.495..705Z | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495..705Z
Constraints on the variation of fine structure constant from joint SPT-SZ and XMM-Newton observations |Bora, Kamal, Desai, Shantanu, | JCAP | 2-12 | 2021 | 2021JCAP...02..012B | http://ui.adsabs.harvard.edu/#abs/2021JCAP...02..012B
A test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers |Bora, Kamal, Desai, Shantanu, | JCAP | 6-52 | 2021 | 2021JCAP...06..052B | http://ui.adsabs.harvard.edu/#abs/2021JCAP...06..052B
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
2013-05-10T08:37:21Z/2013-10-08T00:06:19Z
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 Joe Mohr, 2014, 'Mass calibration of SPT clusters: re-observation of missing pointings', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hqwd96q
