Both X-rays and gravitational lensing are highly recognized paths to carry outcosmological studies, with several space missions being prepared: eROSITA,EUCLIDE, JDEM. Galaxy clusters which are going to be found in all those surveyswill provide a quantum leap in our understanding of the Cosmology. We proposehere a unique path-finder survey optimized for a joint X-ray and gravitationallensing cluster detection in the redshift range of 0.1-1. This proposal is ajoint program on calibrating and extending the 400 square degree survey topursue the measurement of dark energy to 3% accuracy achieved in a combinationwith WMAP, BAO and SN experiments.
Statistical properties of dwarf novae-type cataclysmic variables: the outburst catalogue |Coppejans Deanne L. Kording Elmar G. et al. | MNRAS | 456-4441 | 2016 | 2016MNRAS.456.4441C | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.456.4441C
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
Spectral clustering for optical confirmation and redshift estimation of X-ray selected galaxy cluster candidates in the SDSS Stripe 82 |Mahmoud E. Takey A. | A&C | 16-174 | 2016 | 2016A&C....16..174M | http://ui.adsabs.harvard.edu/#abs/2016A&C....16..174M
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function |Vagnetti F. Middei R. et al. | A&A | 593-55 | 2016 | 2016A&A...593A..55V | http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V
The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey. I. Cluster catalogue and discovery of two merging cluster candidates |Takey A. Durret F. et al. | A&A | 594-32 | 2016 | 2016A&A...594A..32T | http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..32T
A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 |Pons E. Watson M. G. | A&A | 594-72 | 2016 | 2016A&A...594A..72P | http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P
M Dwarf Activity in the Pan-STARRS1 Medium-Deep Survey: First Catalog and Rotation Periods |Kado-Fong E. Williams P. K. G. et al. | ApJ | 833-281 | 2016 | 2016ApJ...833..281K | http://ui.adsabs.harvard.edu/#abs/2016ApJ...833..281K
Searching for gamma-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band |Arsioli B. Chang Y.-L. | A&A | 598-134 | 2017 | 2017A&A...598A.134A | http://ui.adsabs.harvard.edu/#abs/2017A&A...598A.134A
Multiwavelength study of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field |Miyaoka Keita Okabe Nobuhiro et al. | PASJ | 70-22 | 2018 | 2018PASJ...70S..22M | http://ui.adsabs.harvard.edu/#abs/2018PASJ...70S..22M
Constraining the Dark-matter Halo Mass of Isolated Low-surface-brightness Galaxies |Kovacs Orsolya E. Bogdan Akos | ApJ | 879-12 | 2019 | 2019ApJ...879L..12K | http://ui.adsabs.harvard.edu/#abs/2019ApJ...879L..12K
The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey - II. X-ray and optical properties of the cluster sample |Takey Ali Durret Florence et al. | MNRAS | 486-4863 | 2019 | 2019MNRAS.486.4863T | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.4863T
X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field |Ota Naomi Mitsuishi Ikuyuki et al. | PASJ | 72-1 | 2020 | 2020PASJ...72....1O | http://ui.adsabs.harvard.edu/#abs/2020PASJ...72....1O
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
The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters |Pastor-Marazuela I. Webb N. A. et al. | A&A | 640-124 | 2020 | 2020A&A...640A.124P | http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P
Candidate isolated neutron stars in the 4XMM-DR10 catalogue of X-ray sources |Rigoselli Michela Mereghetti Sandro | MNRAS | 509-1217 | 2022 | 2022MNRAS.509.1217R | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.1217R
Constraining X-ray emission of a magnetically arrested disk by radio-loud AGNs with an extreme-ultraviolet deficit |Li Shuang-Liang Zhou Minhua | A&A | 663-4 | 2022 | 2022A&A...663L...4L | http://ui.adsabs.harvard.edu/#abs/2022A&A...663L...4L
The XMM Cluster Survey: an independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies |Turner D. J. Giles P. A. et al. | MNRAS | 517-657 | 2022 | 2022MNRAS.517..657T | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517..657T
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
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 ALEXIS FINOGUENOV, 2012, 'XMM guided survey of the CFHTLS: a Milestone for X-ray Cluster Cosmology', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rhrmabu
