With this proposal we will construct a comprehensive library of X-ray to mid-IRQSO spectral energy distributions for a single epoch (z=1), covering two ordersof magnitude in luminosity. In doing so, we will decouple luminosity effectsfrom evolutionary effects and so determine the amount of radiation that isabsorbed and reprocessed by the torus, and how this depends on luminosity. TheSED library will represent a fundamental resource to reconcile the conflictingresults on AGN obscuration at different wavelengths, and for futureinvestigations of the accretion history of massive black holes. Our SDSS samplehas already been observed in the near and mid-IR with Spitzer; here we requestXMM-Newton observations to provide the UV and X-ray parts of the SED library.
Publications
X-ray Emission from Optically Selected Radio-intermediate and Radio-loud Quasars |Miller B. P. Brandt W. N. et al. | ApJ | 726-20 | 2011 | 2011ApJ...726...20M | http://ui.adsabs.harvard.edu/#abs/2011ApJ...726...20M
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
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
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities |Henley David B. Shelton Robin L. | ApJS | 202-14 | 2012 | 2012ApJS..202...14H | http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H
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
An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission |Henley David B. Shelton Robin L. | ApJ | 773-92 | 2013 | 2013ApJ...773...92H | http://ui.adsabs.harvard.edu/#abs/2013ApJ...773...92H
The 2XMMi/SDSS Galaxy Cluster Survey. III. Clusters associated with spectroscopically targeted luminous red galaxies in SDSS-DR10 |Takey A. Schwope A. | A&A | 564-54 | 2014 | 2014A&A...564A..54T | http://ui.adsabs.harvard.edu/#abs/2014A&A...564A..54T
The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models X-Ray Emission |Henley David B. Shelton Robin L. et al. | ApJ | 800-102 | 2015 | 2015ApJ...800..102H | http://ui.adsabs.harvard.edu/#abs/2015ApJ...800..102H
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
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
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV |Clerc N. Merloni A. et al. | MNRAS | 463-4490 | 2016 | 2016MNRAS.463.4490C | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C
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
Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster |Planck Collaboration Ade P. A. R. et al. | A&A | 596-101 | 2016 | 2016A&A...596A.101P | http://ui.adsabs.harvard.edu/#abs/2016A&A...596A.101P
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
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
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
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
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
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
Diffuse radio emission from non-Planck galaxy clusters in the LoTSS-DR2 fields |Hoang D. N. Bru00fcggen M. et al. | A&A | 665-60 | 2022 | 2022A&A...665A..60H | http://ui.adsabs.harvard.edu/#abs/2022A&A...665A..60H
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 Mathew Page, 2010, 'Decoupling luminosity and evolution in the spectral energy distribution of AGN', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-in56elv
