We propose to complete our 12 deg^2 survey at 50 ks depth of three legacy skyregions\: the SERVS areas of W-CDF-S, ELAIS-S1, and XMM-LSS. XMM-LSS won a 1.3Ms AO-15 allocation. W-CDF-S and ELAIS-S1 coverage is now integrally required sothat XMM-SERVS can dramatically advance studies of SMBH growth across the fullrange of cosmic environments, links between SMBH accretion and host-galaxyproperties, groups/clusters at z = 0.1-2, protoclusters, and other topics.XMM-SERVS will allow outstanding studies of the newly detected 9000 AGNs and 760X-ray groups/clusters by powerfully leveraging its superior radio-to-UVcoverage, and its fields will have extraordinary legacy value as MOONS massivespectroscopy fields, DES/LSST deep-drilling fields, and prime ALMA fields.
The XMM-SERVS Survey: XMM-Newton Point-source Catalogs for the W-CDF-S and ELAIS-S1 Fields |Ni, Qingling, Brandt, W. N., et al. | ApJS | 256-21 | 2021 | 2021ApJS..256...21N | http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...21N
Spectral Energy Distributions in Three Deep-drilling Fields of the Vera C. Rubin Observatory Legacy Survey of Space and Time: Source Classification and Galaxy Properties |Zou, Fan, Brandt, W. N., et al. | ApJS | 262-15 | 2022 | 2022ApJS..262...15Z | http://ui.adsabs.harvard.edu/#abs/2022ApJS..262...15Z
Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth.s Magnetosphere to the Solar Wind Proton Flux |Zhang, Yingjie, Sun, Tianran, et al. | ApJ | 948-69 | 2023 | 2023ApJ...948...69Z | http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z
X-Ray Unveiling Events in a z \\u2248 1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South |Yu, Li-Ming, Luo, Bin, et al. | ApJ | 949-6 | 2023 | 2023ApJ...949....6Y | http://ui.adsabs.harvard.edu/#abs/2023ApJ...949....6Y
Investigating the Star Formation Rates of Active Galactic Nucleus Hosts Relative to the Star-forming Main Sequence |Cristello, Nathan, Zou, Fan, et al. | ApJ | 962-156 | 2024 | 2024ApJ...962..156C | http://ui.adsabs.harvard.edu/#abs/2024ApJ...962..156C
Mapping the Growth of Supermassive Black Holes as a Function of Galaxy Stellar Mass and Redshift |Zou, Fan, Yu, Zhibo, et al. | ApJ | 964-183 | 2024 | 2024ApJ...964..183Z | http://ui.adsabs.harvard.edu/#abs/2024ApJ...964..183Z
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
2018-07-08T23:34:26Z/2020-02-24T05:42:27Z
Version
18.02_20200221_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, Prof William Brandt, 2020, 'Completing and Ensuring Major Impact from the XMM-SERVS Survey', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-7pv1bwb
