GT- This is a survey of magnetic CVs, the goal of which is to determine theiroverall energy balance and, based on the temperature of the X-ray spectrum, themass of the accreting white dwarf for a large sample of objects.
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A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 |Georgakakis Antonis Nandra K. | MNRAS | 414-992 | 2011 | 2011MNRAS.414..992G | http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414..992G
Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog |Georgakakis A. E. Chavushyan V. et al. | MNRAS | 367-1017 | 2006 | 2006MNRAS.367.1017G | http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G
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Detectability of low-energy X-ray spectral components in type 1 active galactic nuclei |Scott A. E. Stewart G. C. | MNRAS | 423-2633 | 2012 | 2012MNRAS.423.2633S | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.2633S
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive |Clerc N. Sadibekova T. et al. | MNRAS | 423-3561 | 2012 | 2012MNRAS.423.3561C | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C
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Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues |Vagnetti F. Turriziani S. | A&A | 536-84 | 2011 | 2011A&A...536A..84V | http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..84V
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A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys |Brightman M. Silverman J. D. et al. | MNRAS | 433-2485 | 2013 | 2013MNRAS.433.2485B | http://ui.adsabs.harvard.edu/#abs/2013MNRAS.433.2485B
Phase-resolved Infrared Spectroscopy and Photometry of V1500 Cygni and a Search for Similar Old Classical Novae |Harrison Thomas E. Campbell Randy D. | AJ | 146-37 | 2013 | 2013AJ....146...37H | http://ui.adsabs.harvard.edu/#abs/2013AJ....146...37H
Phase-resolved X-ray spectroscopy and spectral energy distribution of the X-ray soft polar RS Caeli |Traulsen I. Reinsch K. et al. | A&A | 562-42 | 2014 | 2014A&A...562A..42T | http://ui.adsabs.harvard.edu/#abs/2014A&A...562A..42T
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Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters |Xiao Weike Chen Chen et al. | MNRAS | 432-41 | 2013 | 2013MNRAS.432L..41X | http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X
Do the spectral energy distributions of type 1 active galactic nuclei show diversity? |Scott A. E. Stewart G. C. | MNRAS | 438-2253 | 2014 | 2014MNRAS.438.2253S | http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2253S
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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
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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
Optical spectroscopy of candidates for quasars at 3 < z < 5.5 from the XMM-newton X-ray survey. A distant X-ray quasar at z = 5.08 |Khorunzhev G. A. Burenin R. A. et al. | AstL | 43-135 | 2017 | 2017AstL...43..135K | http://ui.adsabs.harvard.edu/#abs/2017AstL...43..135K
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A Catalog Sample of Low-mass Galaxies Observed in X-Rays with Central Candidate Black Holes |Nucita A. A. Manni L. et al. | ApJ | 837-66 | 2017 | 2017ApJ...837...66N | http://ui.adsabs.harvard.edu/#abs/2017ApJ...837...66N
Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>~1 and their Galaxy Populations |Fassbender Rene | PhDT | 0-116 | 2008 | 2008PhDT.......116F | http://ui.adsabs.harvard.edu/#abs/2008PhDT.......116F
Numerical simulations of high-energy flows in accreting magnetic white dwarfs |Van Box Som Lucile Falize E. et al. | MNRAS | 473-3158 | 2018 | 2018MNRAS.473.3158V | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473.3158V
Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals |Sibeck David G. Allen R. et al. | SSRv | 214-79 | 2018 | 2018SSRv..214...79S | http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S
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The evolving X-ray spectrum of active galactic nuclei: Evidence for an increasing reflection fraction with redshift |Avirett-Mackenzie M. S. Ballantyne D. R. | MNRAS | 486-3488 | 2019 | 2019MNRAS.486.3488A | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.3488A
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline |Hollowood Devon L. Jeltema Tesla et al. | ApJS | 244-22 | 2019 | 2019ApJS..244...22H | http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters |Palmese A. Annis J. et al. | MNRAS | 493-4591 | 2020 | 2020MNRAS.493.4591P | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation |Molham Mona Clerc Nicolas et al. | MNRAS | 494-161 | 2020 | 2020MNRAS.494..161M | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M
Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background |Ananna Tonima Tasnim Treister Ezequiel et al. | ApJ | 889-17 | 2020 | 2020ApJ...889...17A | http://ui.adsabs.harvard.edu/#abs/2020ApJ...889...17A
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
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks |Kosiba Matej Lieu Maggie et al. | MNRAS | 496-4141 | 2020 | 2020MNRAS.496.4141K | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K
SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release |Clerc N. Kirkpatrick C. C. et al. | MNRAS | 497-3976 | 2020 | 2020MNRAS.497.3976C | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C
Multiwavelength Properties of the Newly Discovered Dwarf Nova ASASSN-21kt |Bandeira Victor Lopes de Oliveira Raimundo et al. | RNAAS | 5-182 | 2021 | 2021RNAAS...5..182B | http://ui.adsabs.harvard.edu/#abs/2021RNAAS...5..182B
Low-frequency integrated radio spectra of diffuse steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP |Duchesne S. W. Johnston-Hollitt M. | PASA | 38-53 | 2021 | 2021PASA...38...53D | http://ui.adsabs.harvard.edu/#abs/2021PASA...38...53D
Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT |Yamada Satoshi Ueda Yoshihiro et al. | ApJS | 257-61 | 2021 | 2021ApJS..257...61Y | http://ui.adsabs.harvard.edu/#abs/2021ApJS..257...61Y
Exploring X-ray variability with unsupervised machine learning. I. Self-organizing maps applied to XMM-Newton data |Kovau010deviu0107 M. Pasquato M. et al. | A&A | 659-66 | 2022 | 2022A&A...659A..66K | http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..66K
The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines |Qu Zhijie Koutroumpa Dimitra et al. | ApJ | 930-21 | 2022 | 2022ApJ...930...21Q | http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q
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, Prof Keith Mason, 2008, 'The mass of the white dwarf and physics of the accretion flows in CVs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mzgmbki
